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Page 1: Durham E-Theses Parameters a ecting inductive displacement …etheses.dur.ac.uk/3133/1/3133_1158.pdf · 2014-02-04 · A test coil sensor and signal processing system was designed

Durham E-Theses

Parameters a�ecting inductive displacement sensors

Wilkinson, Michael Richard

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Wilkinson, Michael Richard (2003) Parameters a�ecting inductive displacement sensors, Durham theses,Durham University. Available at Durham E-Theses Online: http://etheses.dur.ac.uk/3133/

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Page 2: Durham E-Theses Parameters a ecting inductive displacement …etheses.dur.ac.uk/3133/1/3133_1158.pdf · 2014-02-04 · A test coil sensor and signal processing system was designed

PARAMETERS AFFECTING INDUCTIVE

DISPLACEMENT SENSORS

Michael Richard Wilkinson

2003

Thesis for the Degree of Master of Science

School of Engineering

University of Durham

= 2 JUN 2004

Page 3: Durham E-Theses Parameters a ecting inductive displacement …etheses.dur.ac.uk/3133/1/3133_1158.pdf · 2014-02-04 · A test coil sensor and signal processing system was designed

Abstract

An investigation of the limitations of inductive displacement sensors (IDSs) was conducted with

the use of electromagnetic finite element analysis (FEA). A comparison of displacement

sensing technologies highlighted the advantages of IDSs in harsh industrial environments, but

an understanding of the operation of IDSs showed that they are limited by the influence of

target material, width and offset. It was proposed that studying the electromagnetic field around

IDSs could reveal more information than was available from the simple impedance

measurements employed by a commercially available lDS.

A test coil sensor and signal processing system was designed and the result was a reliable

system for measuring the magnetic field around the lDS. Experiments showed that the 1 MHz

field had an amplitude of 5 x 10- 6 T at the base of the lDS and two- and three-dimensional FEA

models were constructed that gave closely matching central field values.

The unreliability of the lDS for different target materials was demonstrated experimentally.

FEA simulations showed that changing target permeability and varying target displacement both

altered the whole field amplitude uniformly. This showed that it was not possible to counteract

the target dependence by monitoring the field with the test coil system in this way. Further FEA

simulations revealed field patterns that changed with target offset. An experiment with the test

coil system confirmed that it was possible to use the change in lobe amplitude to measure the

offset of the target; for example when target displacement d1 = 25 mm and offset Os = 1.2 times

the lDS coil diameter, the distance error was 3.6 %, which corresponded to a normalised test

coil output of 0.54. A similar effect was found from target width FEA simulations. Hence it

was possible to correct the output signal from the lDS coil to counteract the effect of an offset

small target.

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Colmtents

Parameters Affecting Inductive Displacement Sensors ................................................................. 1

Abstract. ......................................................................................................................................... 2

Contents ......................................................................................................................................... 3

List of Figures ................................................................................................................................ 5

List of Tables ................................................................................................................................. 8

Declarations ................................................................................................................................... 9

Statement of Copyright ................................................................................................................ I 0

Acknowledgements ..................................................................................................................... I1

Chapter 1 Introduction ............................................................................................................ 12

1.I Non-Contact Spatial Sensors ............................................................................................... I3 1.1.1 Capacitive Sensors .................................................................................................. 13 I .1.2 Optical Sensors ....................................................................................................... 14 1.I.3 Ultrasonic Sensors ................................................................................................... 15 1.1.4 Inductive Sensors .................................................................................................... 16 1.1.5 Comparison of Technologies .................................................................................. I6

I.2 Inductive Displacement Sensor Principles ........................................................................... I7 I.2 .1 IDS Coil Impedance ................................................................................................ 17 1.2.2 The Skin Effect ....................................................................................................... 19

1.3 Inductive Displacement Sensor Applications ...................................................................... 20

1.4 Limitations of IDS ............................................................................................................... 21 1.4.1 Target Material. ....................................................................................................... 21 1.4.2 Target Width ........................................................................................................... 22 1.4.3 Target Offset ........................................................................................................... 22

1.5 Context ................................................................................................................................. 23

1.6 Organisation of the Remainder of this Thesis ...................................................................... 26

Chapter 2 Magnetic Field Measurements ............................................................................... 27

2.1 Magnetic Sensor Technologies ............................................................................................ 27 2.1.1 Low-field Sensors ................................................................................................... 28 2.1.2 Earth's Field Sensors .............................................................................................. 29

2.2 Design Requirements ........................................................................................................... 30

2.3 Magneto-Resistive Sensor ................................................................................................... 32 2.3.1 Amplification Circuit .............................................................................................. 32 2.3 .2 Circuit Testing ........................................................................................................ 34

2.4 Test Coil Sensor ................................................................................................................... 34

2.5 Selection and Refinement of Test Coil ................................................................................ 35 2.5.1 Test Coil Construction ............................................................................................ 36 2.5.2 Test Coil Characterisation ....................................................................................... 37

3

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Contents

2.6 Collection of Data ................................................................................................................ 39 2.6.1 Signal Noise ............................................................................................................ 39 2.6.2 Phase-Locking Program .......................................................................................... 41

2.7 Summary .............................................................................................................................. 43

Chapter 3 Finite Element Analysis ......................................................................................... 44

3. 1 Generalised FEA Modelling Process ................................................................................... 44 3 .1. 1 Setting Up the Simulation ...................................................................................... .45 3.1 .2 Impedance Simulation ............................................................................................. 45 3.1.3 Eddy Current Solver ................................................................................................ 48 3.1.4 Solution Criteria and Meshing ................................................................................ 50

3.2 Two-Dimensional PEA ........................................................................................................ 51 3.2. 1 Test Problem ........................................................................................................... 51 3.2.2 Simulation Refinement ........................................................................................... 54 3.2.3 Parametric Test Problem ......................................................................................... 56

3.3 Three-Dimensional PEA ...................................................................................................... 57 3.3.1 Test Problem ........................................................................................................... 57 3.3.2 Simulation refinement ............................................................................................. 60 3.3.3 Parametric Problems ............................................................................................... 61

3.4 General Considerations ........................................................................................................ 63 3.4.1 FEA of Experimental Equipment.. .......................................................................... 63 3.4.2 Edge Effects ............................................................................................................ 65 3.4.3 Extraction of Data ................................................................................................... 66

3.5 Summary .............................................................................................................................. 68

Chapter 4 Inductive Displacement Sensor Limitations .......................................................... 70

4.1 Target Material .................................................................................................................... 70 4.1.1 Characterising the Effect of Target Material .......................................................... 70 4.1.2 FEA Simulations of the Influence of Target Material... .......................................... 72 4.1.3 Target Material Summary ....................................................................................... 77

4.2 Target Offset ........................................................................................................................ 77 4.2.1 Characterising the Effect of Target Offset .............................................................. 77 4.2.2 FEA Simulations of an Offset Target.. .................................................................... 79 4.2.3 Experimental Measurements of an Offset Target ................................................... 82 4.2.4 Target Offset Summary ........................................................................................... 82

4.3 Target Width ........................................................................................................................ 83 4.3 .I Characterising the Effect of Target Width .............................................................. 83 4.3.2 FEA Simulations of the Effect of Target Width ..................................................... 85 4.3.3 Target Width Summary ........................................................................................... 86

4.4 Summary .............................................................................................................................. 86

Chapter 5 Conclusions ............................................................................................................ 88

Appendix I Published Research ............................................................................................ 91

References ................................................................................................................................... 98

4

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List of Figures

Figure 1.1. Optical displacement sensors with LEDs and PDs. (a) Linear displacement with a second compensating PD. (b) Angular displacement with two main PDs ............... 14

Figure 1.2. The Physical arrangement of an lDS ......................................................................... 17

Figure 1.3. lDS equivalent circuit. ............................................................................................. 18

Figure 1.4. Variation of eddy current properties with depth in the plane wave case. (a) Eddy current density as a function of depth. (b) Eddy current phase angle as a function of depth .................................................................................................................. 20

Figure 2.1. Comparison of typical magnetic field sensor approximate values. Adapted and updated from [29] .......................................................................................................... 27

Figure 2.2. Magnetoresistive effect: a current,/, flows through a ferromagnetic material and an external magnetic flux, B, causes the magnetisation vector, M, to shift by an angle a .................................................................................................................................. 30

Figure 2.3. Amplification circuit used with the MR sensors. Adapted from [33] ..................... 33

Figure 2.4. Constructed amplification circuit with the MR sensor protruding from the left -hand edge ...................................................................................................................... 33

Figure 2.5. Simple test coil construction .................................................................................... 35

Figure 2.6. Magnetic flux density profile of the lDS coil as measured with the test coil. ......... 36

Figure 2. 7. Different coil designs ............................................................................................... 3 7

Figure 2.8. Optimised test coil design. (a) Side view. (b) Projection view .............................. 37

Figure 2.9. Impedance analysis of the test coil. (a) Impedance phase angle 0. (b) Impedance magnitude IZI ..................................................................................................... 38

Figure 2.1 0. Parallel R, L and C circuit model of test coil. ........................................................ 39

Figure 2.11. Signal recorded from a test coil. (a) Global variations. (b) Local variations .............................................................................................................................. 40

Figure 2.12. Screen-shot from the phase-lock Java application ................................................ .42

Figure 2.13. Result of phase-locking an input signal. ............................................................... .42

Figure 3.1. Equivalent circuit for a two-conductor system ........................................................ .46

Figure 3.2. The axial-symmetric geometry of the lDS sensor coil and centred target. Dimensions given in mm ..................................................................................................... 52

Figure 3.3. The magnetic flux plotted for the two-dimensional test problem. The central lighter portions represent a stronger field than the surrounding darker regions .................................................................................................................................. 53

Figure 3.4. Variation in the magnitude of the z-component of the field, IBzl I tesla, with radius, RI mm, along a line 1 mm below the lDS coil. ....................................................... 54

Figure 3.5. Axial-symmetric geometry of the lDS sensor coil and centred target with the inclusion of a dummy object to improve meshing. Dimensions given in mm .............. 55

5

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List of Figures

Figure 3.6. Mesh in the space between the coil and target. (a) The original problem without a dummy object. (b) The problem with a refined mesh inside the dummy object. .......................................... :························································································ 56

Figure 3.7. Magnitude of the z-component of the field, IBzl I tesla, with radius, RI mm, along a line 1 mm below the IDS coil, for a geometry with a meshing dummy object .................................................................................................................................... 56

Figure 3.8. The variation of coil inductance, L, with target displacement, d, ............................. 57

Figure 3.9. Three-dimensional geometry of the IDS coil and non-centred target yz-plane cross-section. Dimensions given in mm .................................................................... 58

Figure 3.1 0. Magnetic flux direction plotted in the yz-plane of the three-dimensional test problem .......................................................................................................................... 59

Figure 3.11. Variation in the magnitude of the z-component of the field, IBzl I tesla, with position y I mm, along a line 1 mm below the IDS coil.. ..................................................... 60

Figure 3.12. Variation in the magnitude of the z-component of the field, IBzl I tesla, with position y I mm, along a line 1 mm below the IDS coil, for a geometry with a meshing dummy object. ....................................................................................................... 61

Figure 3.13. The variation of coil inductance, L, with target displacement, d, for an offset target geometry .......................................................................................................... 63

Figure 3.14. Two-dimensional simulation of the IDS coil and target arrangement with a field-measuring test coil. (a) Magnetic flux plot with stronger field represented by lighter colour. (b) Magnitude of the z-component of the field, IBzl I tesla, with position RI mm, along a line I mm below the IDS coil. ..................................................... 64

Figure 3.15. Two-dimensional simulation of the IDS coil and target arrangement with a plastic target spacer. (a) Magnetic flux plot with stronger field represented by lighter colour. (b) Magnitude of the z-component of the field, IBzl I tesla, with position RI mm, along a line 1 mm below the IDS coil. ..................................................... 65

Figure 3.16. Demonstration of the edge effect on the z-component of the magnetic field around the target. ................................................................................................................. 66

Figure 3.17. Application of the three-dimensional convolution program to the field profile of small-target arrangement. (Solid) raw field. (Dash) Processed field ................. 68

Figure 4.1. Influence of target material on IDS displacement measurements. (Solid) Steel. (Dash) Brass. (Dot) Aluminium. (a) Over the whole measurement range. (b) Close-up to highlight differences ................................................................................... 72

Figure 4.2. Influence of target material on the magnetic field, IBzCz = 3 mm)l. from different target material simulations with d, = 15 mm. R=Omm position is directly below the centre of the IDS coil. (Dash) Steel-1008. (Dot) Nickel. (Solid) Aluminium, copper, brass .................................................................................................... 74

Figure 4.3. Variation in central field value,IBzCr=O, z=3)1. with target displacement, d,. (Dash) Steel-1008. (Dot) Nickel. (Solid) Aluminium, copper, brass ................................. 74

Figure 4.4. Impedance components as a function of target displacement, d,. (Dash) Steel-1 008. (Dot) Nickel. (Solid) Aluminium, copper, brass. (a) Resistance, R. (b) Inductance, L . ................................................................................................................. 7 5

Figure 4.5. Dependence of edge effect on target material demonstrated by the field plotted along a line I mm below the IDS coil. (a) Aluminium. (b) Steel. ......................... 76

6

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List of Figures

Figure 4.6. Influence of target offset on IDS output. Normalised IDS output with target offset, Os, at different target displacements, d,. (Solid) d, = 10 mm. (Dash) d, = 20 mm. (Dot) d, = 30 mm ............................................................................................ 78

Figure 4. 7. Field profiles for large offset targets for d, = 10 mm. (Solid) Os = 0 mm. (Dash) Os= 100 mm. (Dot) o., = 100 mm. (Dash dot) Os= 125 mm. (Dash dot dot) 0 5 = 125 mm ......................................................................................................................... 79

Figure 4.8. FEA simulations of offset targets at different target displacements. (a)- (d) d, = 10 mm. (e)- (h) d, = 30 mm ........................................................................................ 81

Figure 4.9. Influence of target offset on coil inductance. (Solid) d, = 10 mm. (Dash) d, = 20 mm. (Dot) d, = 30 mm ............................................................................................ 81

Figure 4.1 0. IDS coil impedance and magnetic field lobe amplitude ford, = 30 mm. (Left, solid) Lobe amplitude. (Right, broken) IDS coil inductance .................................... 82

Figure 4.11. Experimental confirmation of FEA simulation results. (Left, solid) Normalised test coil signal. (Right, broken) IDS distance error. ....................................... 82

Figure 4.12. Influence of target width on the IDS output. .......................................................... 84

Figure 4.13. Influence of target width on the IDS output. (Solid) w, = 2.6. (Dash) w, = 1.4. (Dot) w, = 1.2. (a) Non-linearity introduced with different target widths. (b) Distance measurement error resulting from small target widths .................................... 84

Figure 4.14. FEA simulations of the influence of target width on the magnetic field. (a)- (d) d, = 10 mm. (e)- (h) d, = 20 mm .......................................................................... 86

7

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List of Tables

Table 1.1. Example applications for ID Ss .................................................................................. 21

Table 3.1. Parameters taken by macro from project file name, where d, = target distance, w, = target width, o5 = target offset. ..................................................................................... 62

Table 4.1. Physical properties of some targets investigated ....................................................... 71

Table 4.2. Influence of target material on IDS coil impedance .................................................. 76

8

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Declarations

The author confirms that this thesis conforms to the word length prescribed for the degree to

which it is submitted.

No part of the material offered in this thesis has been previously submitted by the author for a

degree in this or any other University.

9

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The copyright of this thesis rests with the author. No quotation from it should be published

without prior written consent and information derived from it should be acknowledged.

10

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Acknowledgements

The support and continuously optimistic encouragement from my supervisor Sherri Johnstone

has been very much appreciated and has been pivotal to the success of this work. Many thanks

are also extended to Dave Wood for his assistance throughout the project.

11

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Chapter 1

Introduction

The sensor industry is a diverse one, yet it is vital to almost all modem manufacturing processes.

Continual sensor research and development is required to meet the needs of industry by

providing innovative solutions to increase reliability and decrease costs. The field encompasses

research into a range of technologies including optical, ultrasonic and biological for functions

such as liquid and gas sensing, displacement measurement, tomography and water quality

monitoring. Industry sectors where applications are found are just as diverse and include the

automotive industry, structural monitoring for civil and aerospace structures, the chemical

industries and the food industry [ 1].

In many industrial locations - for example in steel works and on production lines - the

distance to metallic materials often needs to be measured and monitored. This task can be

difficult when the application environment is dusty, steamy or similarly harsh. Inductive

proximity sensors are appropriate for this type of situation because they rely on electromagnetic

fields that can pass through the intervening medium unaffected. This type of sensor is now

common place in harsh industrial environments, so the exploration of their limitations and

subsequent improvement is an important physical problem.

This thesis summarises research performed in this important area and in this first chapter the

topic is introduced. There are a number of different technologies suitable for non-contact

displacement measurements and here capacitive, optical, ultrasonic and inductive sensors are

discussed (§ 1.1 ). Their applications and relative merits are observed with particular reference

to the harsh industrial environment described above. This gives a justification to the particular

importance of inductive proximity sensors, which are introduced through a discussion of their

operating principles (§ 1.2) and applications (§ 1.3). The basis of this work has been the

investigation of the limitations of these sensors through research into the influence of target

material, offset and width, which are introduced in section § 1.4. The wider context of this

work and its relation to previous research and publications is discussed (§ 1.5) before the

chapter concludes with a discussion of the organisation of the remainder of this thesis (§ 1.6).

12

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Chapter 1

1.1 NonaContact Spatial Sensors

There are number of spatial measuring devices that are useful in an industrial context and they

may be classified as proximity, position, displacement, dimension and vibration sensors. Often

a non-contact spatial sensor can operate in a number of these modes depending on how it is

installed. Proximity sensors return an on or off output signal denoting presence (or part

presence) or absence of the target. Position sensors record the location of an object with respect

to a defined reference coordinate. Displacement sensors give the movement from one position

to another in a defined direction. Part specific geometrical measurements can be determined

with dimension sensors. Finally, the amplitude and frequency of targets with oscillatory motion

are commonly measured with a vibration sensor. The advantage of non-contact sensors over

contact-based sensors is that there is no risk of damage to fragile parts and the sensor can be

positioned in a convenient location to avoid interference with the process being measured.

Industrial processes often require the use of these non-contact spatial sensors to monitor the

target objects in a number of applications from robotic positioning systems to quality control.

Such instruments operate using capacitive, optical, ultrasonic or inductive technologies [2] [3].

Each type has its own set of characteristics and the particular sensor used will depend on

considerations such as: the motion and degrees of freedom to be measured e.g. rotational or

linear motion in single or multiple dimensions; the operating environment e.g. temperature,

humidity, dust, vibrations or mechanical shocks; the required measurement range; and the

measurement performance e.g. sensitivity, linearity and accuracy requirements.

1.1.1 Capacitive Sensors

The capacitance of a pair of electrodes is given by the basic formula C = E G where c is the

permittivity of the dielectric and G is a geometrical factor. For a parallel flat plate capacitor

G = A/ d where A is the area of the plates and d is the displacement between them.

Capacitance-based non-contact spatial measuring systems consist of a sensing plate positioned

above a conducting target and a potential difference developed between the two enables

measurement of the capacitance. Such a system can be constructed in a similar manner to a

variable capacitor, whereby the overlap between the plates, and therefore A, changes depending

on the angular position of the target. This gives an angular position sensor. Alternatively, and

more commonly, if the device is assembled such that d changes with the displacement to be

measured, then the result is a simple, but linear, non-contact displacement sensor. Devices can

be constructed to cover a measurement range of about 2.5-250 mm [3].

Capacitive transducers are also sensitive to changes in the material between the sensor plate

and the target; therefore maintaining a constant dielectric permittivity is important. The

13

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Chapter 1

dielectric constant of air increases with humidity and is also influenced by other materials such

as dust, dirt, oil etc. in the sensing gap. This affects the capacitance and thus the resulting

distance measurement. Thermal expansion and contraction of sensor components is a further

source of error and this is a substantial problem when measuring or controlling to high

precisions.

1.1.2 Optical Sensors

Light-emitting diodes (LEDs) and photodiodes (PDs) have fast responses to current and light

intensity respectively, which makes them suitable for use in an intensity-based optical

displacement sensor. Figure l.l(a) shows how an LED and a PD can be positioned face on to

each other to measure the distance between them. A second PD can be added to compensate for

ambient illumination levels and LED fluctuations. Alternatively an angular displacement sensor

may be composed from two fixed position PDs and a moveable LED (figure l.l(b)).

Measurement errors are reduced by combining and averaging the signals from the two PDs. To

further reduce the influence of ambient illumination, the incident light may be modulated and

phase-locking signal processing used to decode the signals from the detector.

Compensator PD (fixed position)O

LED Main PD

(fixeld posl~~l-o-n) ______ (p_o_s-it-io~."Fchanges)

Distance measured

(a)

PD (:)xed position)

Angle measured

aD r--1_ __ t \...._.:.:.! = = = - -.. LED (angle changes)

(fixed position)

(b)

Figure 1.1. Optical displacement sensors with LEDs and PDs. (a) Linear displacement with a second compensating PD. (b) Angular displacement with two main PDs.

Other mechanisms, such as that developed by Wang [4], use light reflected from the target to

obtain a displacement measurement. As the reliability of laser diodes has increased, laser-based

systems are now available that also use a reflection mechanism. The radiation from laser diodes

can be of a much higher intensity than ambient light and so background effects are reduced.

However, all optical systems are most obviously limited by the need for a clean measurement

gap; intervening dust, oil, metal filings, etc. will reduce the reliability of the measurement.

14

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Chapter 1

1.1.3 Ultrasonic Sensors

The term ultrasonic refers to sounds with frequencies greater than those audible to humans,

which usually incorporates frequencies greater than 20 kHz. Although medical scanners use

frequencies in the range 1 - 20 MHz, ultrasonic spatial sensors typically utilise the range 20 -

200 kHz. Such devices emit a short burst of ultrasonic sound towards a target, which is then

reflected back to the sensor. The time between transmission and reception of the burst gives a

value for the distance between the sensor and the target. This technology is well established and

a wide range of sensors are available which operate at different frequencies and have different

radiation patterns. The resolution of the measurements depends on the wavelength of the sound

emitted by the sensor, but in general, commercial products are available with resolutions in the

range 0.2- 0.7 %of the full scale.

Assuming transmission occurs under adiabatic conditions, the speed of sound, c, is a function

of temperature, T, and varies as

c=~r:r ( 1.1)

where y is the ratio of heat capacities, R is the universal gas constant(= 8.314 J.mol- 1 .K- 1) and

m is the molar mass of the transmission medium. If it is assumed that air is a diatomic ideal gas

(y= X) with a molar mass of 29.0x10- 3 Kg.mol- 1, then at T=273.15K (0°C),

c = 331.1 m.s- 1• For the higher temperature of T = 313.15 K ( 40 °C), the speed is increased to

c = 354.5 m.s- 1• This demonstrates the requirement for effective temperature compensation.

The nature of the medium in which the ultrasonic system is operating must also be taken into

consideration. In a non-dispersive medium- such as air- the frequency has no influence on

the speed of sound and the energy and sound travel at the same speed. In a dispersive medium

- such as water - sound speed is a function of frequency and each frequency component

propagates with its own phase velocity, but the energy travels at the group velocity.

The maximum range of these sensors depends on the attenuation of the sounds waves. In air

the attenuation of the ultrasonic pulse increases with the frequency and for each frequency the

attenuation is a function of humidity. Industrial processes in the sensor environment may

produce background noise in the ultrasonic range. However, in general, this is less likely to be

a problem at higher frequencies. The size and form of the target affects the intensity of the

reflected sound burst. A large flat surface will reflect the whole beam and the received intensity

is equivalent to the intensity at twice the target distance. An example of this type of situation is

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Chapter I

measuring the level of a large vat of still liquid. When the target is not flat, a reflection

coefficient may be calculated, which can be taken into consideration when selecting the sensor.

1.1.4 [nductive Sensors

There are two main types of inductive displacement sensor (IDS): those with one coil and those

with more than one coil [2]. IDSs with two or more windings generally consist of a

transmission coil and one or more receiver coils. A conducting material positioned between the

coils will result in a change in the flux measured by the receiving loop. The general

configuration is to have two coils facing each other with a conducting bar that is free to move

between them. Thus by moving the conducting bar and monitoring the receiving loop

impedance, a displacement can be determined. This type of sensor has been utilised in a

number of applications for example by Bartoletti et al. [5] who use such a device in a low-noise

accelerometer for the detection of gravitational waves.

The second type of inductive sensor with one coil can be utilised for non-contact

displacement measurements. Such devices generally comprise a main sensor coil from which

distances are measured and an oscillator I demodulator electronic module as shown in figure 1.2.

The output of the system is a voltage that is directly proportional to the distance being measured.

This type of sensor is used widely in the measurement of the distance to conducting targets in

harsh environments because they are not affected by dust, dirt, humidity etc. between the sensor

and target and because they can be enclosed in a protective casing to allow operation at high

temperatures.

1.1.5 Comparison of Technologies

The technologies of capacitance, optical, ultrasonic and inductive displacement sensors have

been discussed and their relative merits and shortcomings offered. In the context of a harsh

industrial environment - where the measurement gap may be inconsistent and contaminated

with particles of dust, oil, etc. -it is apparent that eddy current inductive displacement sensors

are the most useful. Capacitance-based sensors are limited by their dependence on the

permittivity of the dielectric between the sensing plate and the target material. A more detailed

comparison between capacitive and inductive sensors is offered by Welsby [6]. Although laser­

based optical displacement sensors offer an increased reliability compared to LED and

photodiode systems, they are still limited by particles in the sensing gap. IDSs are well suited

for harsh environments, but this type of sensor is not without limitation and the work presented

here has focused on these devices and research into improving them.

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Oscillator and demodulator Voltmeter

;::::~::::::=.::f------- lDS coil in protective housing

Conductive target material

Figure 1.2. The Physical arrangement of an IDS.

1.2 Inductive Displacement Sensor Principles

Chapter 1

Figure 1.2 shows how an alternating current, / 1, passes through the IDS coil to generate an

alternating magnetic field, H 1• When a conducting target is positioned in the field, eddy

currents are generated on the surface and this produces a secondary magnetic field, H2, which

opposes H 1•

1.2.1 IDS Coil Impedance

The equivalent circuit of the IDS system consists of two loops: the IDS coil and the induced

eddy currents in the target. This arrangement is shown in figure 1.3. A change in the current of

loop one results in a change in the flux through that coil. Loop one and loop two are

magnetically coupled and so a potential difference is induced in the target material. The

induced voltage, V2, is proportional to the rate of change of the flux and thus the rate of change

of the current in loop one, / 1, such that

V - M dl! 2-- I2d/ ( 1.2)

where M 12 is the coupling constant between loop one and loop two, called the mutual inductance,

which depends on the geometrical arrangement of the IDS coil and the target. M21 can be used

to quantify the magnetic coupling between loop two and loop one. In general these two mutual

inductances are equal since loop one and loop two may be interchanged without affecting the

mutual inductance. Thus the mutual inductance is

M =MI2 =M2I ( 1.3)

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Loop I (IDS coil)

Loop 2 (target)

Figure 1.3. lDS equivalent circuit.

Chapter I

Figure 1.3 shows that each loop has an inductance (L 1 and~) and resistance (R 1 and R2). The

potential difference across the sensor coil with a current of angular frequency, w, is given by

Kirchoffs voltage law as

(1.4)

where i = ~ . But for the second loop there is no overall potential difference and so

(1.5)

Combining these two equations gives an expression for the potential difference across the IDS

coil

( 1.6)

from which the IDS coil equivalent impedance can be extracted

(1.7)

This leads to frequency dependent equations for the IDS coil equivalent resistance

(1.8)

and equivalent inductance

(1.9)

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Chapter 1

1.2.2 The Skin Effect

An important result of the flow of eddy currents in the target material is the skin effect. This is

the tendency of eddy currents to concentrate in the surface of the target closest to the excitation

field. As the frequency of the excitation field increases, the skin effect increases and the

currents become more concentrated at the surface. The effect is also dependent on the target

conductivity and permeability. The amplitudes of the currents decrease exponentially - or

approximately exponentially, depending on the geometry of the material- with depth into the

target. Also with increased depth, the phase difference between the currents at that depth and

the surface currents increases. An explanation of the skin effect is that eddy currents produce a

magnetic field at a greater depth that counteracts the excitation field, thus reducing its ability to

generate eddy currents deeper in the material.

Libby [7] (pages 123-135) shows that in the plane wave case, where a target of infinite extent

is impinged upon by a perpendicular field of infinite extent, the current density Jz, at a depth z,

is given by

(1.10)

where 10 is the surface current density, f is the frequency and f1 and a are the permeability and

conductivity of the target material respectively. For non-magnetic materials the permeability is

that of free space, f1 = flo = 4rr x 10- 7 H.m- 1, otherwise f1 = flo flr where flr is the relative

permeability of the material. A factor called the standard depth of penetration, or skin depth,

can be introduced that is the depth where the current density has decreased to )!; times its value

at the target surface. Therefore ( 1.10) may be written as

(1.11)

where 8 = (;r f flCY rx is the standard depth of penetration. Figure 1.4(a) shows this variation of

eddy current density with depth into the target. The axis of abscissas has the depth relative to

the standard depth of penetration and the axis of ordinates has the current density relative to the

surface current density.

The phase difference in radians, B, between 10 and Jz is given by

z (1.12) =

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Chapter I

Figure 1.4(b) show a plot of the phase Jag with depth into the target material. The axis of

abscissas has the depth relative to the standard depth of penetration and the axis of ordinates has

the phase difference between lx and 10•

0.8

0 0.6 ...., -....;· 0.4 .

0.2

0 2

(a)

3 4 5 6 z I r5

6

4 "1:1 e -"' 2

0

0 3 4 5 6 z I r5

(b)

Figure 1.4. Variation of eddy current properties with depth in the plane wave case. (a) Eddy current density as a function of depth. (b) Eddy current phase angle as a function of depth.

1.3 Inductive Displacement Sensor Appli.cations

IDSs may be used in a wide variety of applications ranging from simple distance measurement

to vibration alarms. The electromagnetic nature of IDSs means that they are not affected by

dust, humidity, etc. and may be employed in applications where other technologies - such as

ultrasonic sensors -are not appropriate. Some example applications are detailed in table 1.1.

Aknin et al. [8] describe the use of an IDS in the railway industry for the measurement of the

relative lateral displacement of a rail/wheelset or rail/bogie. Specific applications given are:

"the measurement of the track gauge at high speed, the measurement of the yaw angle and

lateral motion of a bogie, and finally the active steering of the railway wheelset". The device

was expected to operate with rain, frost, snow, rapid cooling of the device when entering

tunnels, large acceleration forces and the possibility of one side being heated through sun

exposure and the other remaining cool in shadows. Optical sensors were ruled out because of

mud, chips, metal filing and grease splashes, and capacitive sensors were unfeasible because of

the large displacement that was required to keep the sensor clear of guard rails, level crossings,

etc. Hence an IDS array was found to be the most suitable system.

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Chapter 1

Table 1.1. Example applications for IDSs.

Application

Alignment

Cylinder diameter

Non-conductive material thickness

Part sorting

Vibration measurement or alert

Description

Two IDSs positioned perpendicularly around a joint can be used to show the position of a metallic rod during an alignment process.

Two IDSs diametrically positioned towards the cylinder (e.g. a shaft) can be used to measure the diameter if the separation of the IDSs is known first.

Place the test material on a conducting base and the ECS on the upper side of the material.

Metallic parts on a conveyor system can be sorted by their height over the surface.

Both the amplitude and frequency of vibrations in a metallic object can be recorded. The maximum frequency will be limited by the response times of the electronics and the operation frequency of the coil.

An inductive proximity sensor is described by Sharp and Pater [9] for use in a nuclear facility

to provide status information on moving machinery. Although this paper refers specifically to

proximity sensors rather than displacement sensors, the same principles are applicable. The

authors describe the benefits of using these sensors in a nuclear facility where the reliability of

remote sensing equipment has important safety implications. Although standard inductive

sensors are generally reliable, when subjected to ionising radiation they can fail at relatively low

and unpredictable total doses. By redesigning the electronic circuit and selecting cables with

appropriate specifications, a sensor with radiation tolerance was developed. The tested sensor

has been manufactured by AEA Technology and has found applications in the thermal oxide

reprocessing plant at Sellafield. Some further applications of IDSs are given towards the end of

this chapter in section § 1.5.

1.4 Limitations of lDS

Eddy current IDS have a number of limitations and it is the purpose of this thesis to discuss

these restrictions on their reliability and applications. Section § 1.2 has introduced the theory of

operation for IDSs, which forms the basis of why target material affects the output of the sensor.

Other factors affecting the reliability of IDS measurements are the target width and target offset.

These factors place important limits on the range of applications in which IDSs can be

employed.

1.4.1 Target Material

Equation ( 1.7) shows that the equivalent impedance, Z, of the sensor coil depends on the

angular frequency, w, and thus the frequency, f, of the current 11• The resistance of the eddy

current path, R2, is a function of the resistivity of the target, p, and inductance of the target

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Chapter 1

depends on the permeability of the target, Jl. Also, as mentioned in section § 1.2, the mutual

inductance, M, varies with the geometry of the coil and target arrangement and so it is a

function of the target displacement from the IDS coil, d,. Thus Z is a function of all these

factors, i.e.

(1.13)

For eddy current displacement sensors, f. p and J1 must be controlled to give the single variable

function

z = g(d,) (1.14)

The frequency may be controlled by selecting a suitable value at the design stage that will

depend on the target skin depth as described in section § 1.2.2. However, p and J1 are properties

of the target material and vary between, for example, steel and aluminium (see table 4.1). This

target dependence can be a major limitation of an eddy current IDS and in situations where

different targets need to be measured, the IDS needs to be recalibrated each time. Commercial

IDSs are usually optimised for either magnetic or non-magnetic targets and it is difficult to use a

system tuned for non-magnetic materials with a magnetic target. Indeed manufacturers state

that with some smaller sensors it is impossible to use a mismatched target and system as the

electronic circuits are optimised for the specific application.

1.4.2 Target Width

The ratio of target size to sensor coil diameter is an important consideration when selecting an

lDS system. Sensor coils can be either shielded or unshielded depending on the application; the

flux from unshielded sensors tends to extend laterally beyond the coil diameter, whereas the

flux from shielded sensors does not tend to spread out in this way. The linear measuring range

is directly proportional to the sensor coil diameter with unshielded coils having a greater

measuring range than shielded coils. A manufacturer's IDS operation manual [ 1 0] states that

for shielded sensors the target should be a minimum of 1.5-2 times the coil diameter, whereas

for unshielded sensors the target material must be at least 2.5-3 times the coil diameter. Using

an IDS with targets smaller than the specified widths will lead to degradation in linearity and

long-term stability. However a target of size greater than the required minimums does not affect

the system.

1.4.3 Target Offset

The influence of an offset target, that is a target that is displaced laterally relative to the centre

of the IDS coil, is related to that of target width. When a target is offset, it appears to be smaller

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Chapter I

than the required width on the side which has been moved towards the centre of the coil. This

situation can arise where either the target has moved off-centre or the lDS coil has been

displaced laterally.

1.5 Context

lDS technology is well established and much of the current research is based in the sensor

manufacturing industry. For this reason trade journals can provide a useful insight into the

current market and commercially available technologies. For example, an introduction to these

sensors is presented by Welsby and Hitz [ 11] and the techniques required to design and build an

eddy current lDS are given by Roach [ 12]. Besides this, there are also a number of published

works that detail the modelling and improvement of IDSs, from which principles and theories

can be extracted and applied to the work in this thesis.

The inhomogeneity resulting from different target materials is a major problem although only

a small quantity of research on this matter has been published, such as that presented by Tian et

al. [13] and Wang and Becker [14]. In the Tian et al. paper, the influence of target resistivity

and permeability are investigated, as is the influence of the converting circuits. The work

concludes, " ... the effect of inhomogeneity in non-ferrous targets is much less than that of

ferrous targets. Therefore non-contact displacement eddy current sensors are suited to

applications for the precision measurement of non-ferrous targets." Wang and Becker have

reported on their design of an lDS that gives a displacement that is described as being

"practically independent of the material of the object".

There have been a number of reports of new designs and applications of IDSs, such as

Passeraub et al. [15] who present a system that utilised a flat coil to achieve sub-micrometric

sensitivity.

Research published by Bartoletti et al. [5] details "the design of a proximity inductive sensor".

The aims of the work were to get low dimensions, a fast response to change in target

displacement and low costs. The proximity sensor used flat coils that were constructed from a

spiral design etched on a double-sided copper printed board. The advantage of this cheap

process was that the coils were very thin and could therefore be placed in close proximity to the

target. This was found to lead to greater sensitivity compared to the more usual design that

extends laterally relative to the plane of the coil. The paper gives a qualitative discussion about

the temperature dependence of their sensor, which is relevant to the work in this thesis; although

the Bartoletti et al. descriptions are complicated by the fact tat they have used spiral coils.

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Chapter I

Macovschi and Poupot have presented a two stage report on their study of variable inductance

transducers as proximity sensors. The first part [ 16] describes the computer simulations of the

magnetic circuits in a coil and target system, which were used to extract magnetic parameters.

The magnetic field, the geometry and position of the coils, the permeability of the magnetic

circuits and targets and the saturation of the magnetic circuits were studied. The simulations

were used to compare two different coil core designs and in the second part [ 17] one of the

designs was selected for experimental investigation. Results were presented for the variation of

coil inductance with a number of parameters including: position and geometry of the coils,

magnetic circuit material, target thickness, coil frequency and some auxiliary construction

elements.

A highly sensitive and compact sensor system utilising 1 mm diameter coils has been

demonstrated by Passeraub [18]. The system also incorporated a new electronic interface that

was surface-mounted onto a PCB to include short leads and a low component count. The result

was a low-noise, high-sensitivity lDS. To demonstrate the system, it was used to control a

stepper motor by detecting a 1 mm hole drilled in a rotating brass disc. This was shown to

permit a well-defined numbering of the motor's steps and hence enabled more control of the

motor.

Much work has been done to utilise eddy current -type sensors to measure profiles and

outlines of metallic objects in a process called electromagnetic tomography. Peyton et al. [19]

present an overview of this method, which includes operating techniques and some examples.

Hardy et al. [20] used an eight by eight array of spiral coils to detect and recognise metallic

objects. Each coil was an eddy current lDS and the 64 elements gave a total sensing area of

320 x 320 mm. The output of the system was a computer image which was used to identify

metallic objects in the sensing range. Fenniri et al. [21] used an eddy current lDS to measure

the distance to a conducting target and then utilised a deconvolution algorithm to extract the

profile of the target surface. The system was only demonstrated for certain targets, although

Fenniri et al. suggest that it could have been employed to make an image of simple-shaped

profiles such as toothed gearings, which would allow for the detection of fractured edges. On

similar lines, Passeraub et al. [22] utilise their highly sensitive small coil IDSs to determine

metallic profile and material information of coins. They demonstrate their system by

highlighting the difference in results from genuine and fake coinage.

Belloir et al. [23] describe a smart flat-coil eddy current sensor for metal tag recognition used

to identify buried pipes. The tags were buried with utility pipes and nine configurations were

used to give a unique identification to the utility type (e.g. water, gas, data cabling, etc.). The

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Chapter 1

intention was that workers were able to locate and identify pipes without needing to excavate

investigation trenches. Although separate emission and receiving coils were used, this work is

closely related to eddy current IDSs in that the metal tags affected the flux distributions such

that they could be identified remotely. The system was further improved [24] and the authors

state that they have reduced the risk of tag misidentification to nearly zero. This work gives

useful insights into hardware and signal processing considerations for IDSs.

An interesting application of an IDS is to measure the position of diesel engine valves as

presented by Marcic [25]. Previous work had involved fitting a sensor to the valve, which

altered its mass and therefore affected the measurements being taken. However, Marcic's

system uses two coils fitted around the valve that do not interfere with its operation. This is not

an eddy current based IDS, but again the design processes given in the paper are relevant to the

present work.

In Scarr and Zelisse's work [26] an eddy current system is used to measure the thickness of

metallised films. The system relies on the skin effect in the target material to attenuate the

incident flux. Results were obtained using just one coil and this operated in a similar manner to

that described here in section § 1.2 and gave a response to target displacement as well as target

thickness. However Scarr and Zelisse wanted a system that would provide thickness results

independent of the target position. To realise this, two coils were used and the target material

was positioned between them; one coil acted as a transmitter and the other as a receiver. The

authors also describe a system where the two coils are on the same side of the target, with the

receiver wrapped inside the transmitter.

On the subject of modelling magnetic displacement sensors, J ohnstone and Peyton [27]

describe the use of three-dimensional finite element simulations to evaluate the performance of

a magnetic sensor system. The technique of using a quarter-geometry model is described and

compared to the full geometry model. Methods to overcome problems associated with meshing

errors are described and the model results are compared to experimental measurements. The

system described by Johnstone and Peyton is quite different from the IDSs described in this

thesis, although the paper's description of the modelling is useful. Huang et al. [28] have also

used finite element analysis to model a displacement sensor. The paper describes how a three­

dimensional model of two coils from a non-contact inductive system was constructed. The

models helped the authors to understand the non-linear nature of the device and assisted in the

optimisation of the design.

In summary, despite IDSs now being off-the-shelf devices, research continues m design

optimisation, miniaturisation and the investigation of new applications. Related work on finite

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Chapter 1

element analysis provides a useful insight into the techniques required to produce reliable

models of IDSs. There has been some investigation of the limitations of IDSs although these

issues have not been fully resolved and still remain an important area ofresearch.

1.6 Organisation of the Remainder of this Thesis

In this chapter the subject of IDSs has been introduced and compared to other sensor

technologies. The performance of these different sensors in a harsh industrial environment has

been discussed and it is argued that IDSs are most appropriate for measuring distances when the

sensing gap is contaminated with dust, steam or oil, etc. Some general applications of lDS have

been introduced and some specific applications have been given. A discussion of the physics of

lOSs has been given, which not only presented an understanding of their operation, but also

described why they are limited by their dependence on the target material. The other limitations

discussed were the influence of target width and target offset. Finally there was a presentation

of some references to previous published research on the subject of lDS applications and

improvements, which sets this thesis in context.

It has been demonstrated that IDSs measure changes in their coil impedance and use this to

determine the target displacement. It is the total field that affects the impedance and therefore

local variations are neglected. The central contention of this thesis is that the structure of the

field can reveal information that is not available from these simple impedance measurements.

The remainder of this thesis describes research that confirms this hypothesis as axiomatic and

utilises this information to address the current limitations of IDSs. Chapter two describes how

measurements of the lDS magnetic field were made. A number of technologies were

investigated and the most appropriate was selected for use in the subsequent experimental work.

Chapter three shows how finite element analysis simulations were used to model the lDS and

includes a discussion of the merits and applications of two- and three-dimensional schemes.

The fourth chapter shows the results of experimental and practical work on the limitations of

lOSs resulting from target material, target offset and target width. The final chapter forms a

summary of the work and draws conclusions about the practicability of making improvements

to lDS designs.

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Chapter 2

Magnetic Field Measurements

Magnetic fields are central to the operation of IDSs and in this chapter methods for taking

measurements of these fields are described. Magnetic sensing technology has a broad range in

terms of both field strength and the physics involved; this was researched and the relative merits

of different sensors were compared. An estimate of the field amplitude and frequency was

made, which enabled suitable measurement devices to be identified. The application of both

magneto-resistive and test coil devices was investigated and the most appropriate was selected.

Signals were recorded using a digital oscilloscope and a Java application was developed to

reduce the noise using a phase-locking technique. The result was a system that was appropriate

for the field range and frequency of the IDS and this was subsequently applied to the

experimental work described later in this thesis.

2.1 Magnetic Sensor Technologies

Magnetic Sensor Technology

Search Coil

Flux Gate

Optically Pumped

Nuclear-Precession

SQUID

Hall-Effect

Magnetoresisti ve

Detectable Field IT

10 I~ 10 -~ 10 4

I.~ZL ... ~=-~:~\FC:::~::::;::.

.... ,, __ • ~:..:::. ilk'>.~.'--·

Figure 2.1. Comparison of typical magnetic field sensor approximate values. Adapted and updated from [29].

A variety of devices can be used to detect magnetic fields and the technology involved

determines whether they are classified as low-, medium-, or high-field sensors [30]. Devices

that detect magnetic fields < - 10- 10 T can be described as low-field sensors. Given that the

magnitude of Earth's field is - 5 x 10- 5 T, medium-field sensors which operate in the range

10- 10- 10- 3 T, are referred to as Earth's field sensors. Detectors that measure fields > 10- 3 T

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Chapter 2

can be labelled as bias magnet field sensors. Figure 2.1 lists some devices and their associated

typical approximate sensing ranges.

2.1.1 Low-field Sensors

It can be seen in figure 2.1 that a variety of low-field sensors exist. Application areas include

measuring the nemo-magnetic fields in the brain and military surveillance equipment. However,

these devices tend to be costly and bulky compared to other magnetic field sensors that are

suitable for detecting stronger fields. It should be noted that the fields that are measured by

these sensors are much less than Earth's field and so careful design choices must be made to

ensure that the field of interest is preserved on the output signal. Some technologies suitable for

measuring in this range are nuclear precession magnetometers, superconducting quantum

interference devices and test coils.

Nuclear-Precession

Nuclear-precession magnetometers generally consist of a hydrogen-rich core surrounded by a

coil. Current is passed through the coil to generate a DC magnetic field that aligns the spinning

protons (hydrogen nuclei) like dipole magnets along the direction of the field. After the coil is

turned off the protons are only subject to the magnetic field that is being measured. This field

causes torque on the spinning nuclei and they precess around the direction of the field.

Consequently a small alternating current is induced in the coil with a frequency equal to that of

the precession. Since the field strength is proportional to the precession frequency, an accurate

value for the magnetic field can be determined. Although this type of device can measure very

low fields, it was deemed impractical for the application in hand. The same is true of optically

pumped and fibre-optic magnetometers.

SQUIDS

Superconducting quantum interference devices (SQUIDs) [31] can detect magnetic fields over

15 orders of magnitude from several teslas to several femto-teslas. First developed in the early

1960s these devices utilise a J osephson junction and until recently required low temperatures to

operate. Low temperature superconducting systems are not well suited to practical use outside

the laboratory because of the sophisticated and ex pensive liquid helium (- 4 K) cryogenics

involved. However with the advent of (relatively) high temperature superconductor thin films

SQUIDs have become more practical for testing purposes since they only require smaller and

cheaper liquid nitrogen cooling (- 77 K). Indeed the use of such high temperature SQUIDs has

been demonstrated for enhancing eddy current non-destructive investigation of metallic

structures [31]. However practical and low cost off-the-shelf SQUID systems are a long way

off.

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Chapter 2

Test Coils The list in figure 2.1 shows that test coils have a wide sensing range and can be used to measure

low-fields. When a loop of wire is subject to an alternating magnetic field, Faraday's law of

magnetic induction states that the EMF of the loop is equal to the negative of the rate of change

of the magnetic flux through the area enclosed by the loop. For a coil of multiple loops, the

EMF is simply multiplied by the number of turns. This is the basis of search coil magnetic field

sensors. The sensitivity depends on the number of loops, the coil area and the permeability of

the core. Since these devices rely on changing magnetic fields - or moving through one -

they cannot be used to measure static or slow-varying fields.

2.1.2 Earth's Field Sensors

Given their sensing range, sensors m this group are typically used to measure the Earth's

magnetic field. Example applications include using electronic compasses for navigation,

determining the yaw of aircraft and projectiles and measuring variations in the field for road

traffic measurements. Some technologies that fall into this range are fluxgate, magnetoresistive

and Hall-effect sensors.

Fluxgate Fluxgate sensors [32] can be used to measure DC or low frequency AC magnetic fields over the

range 10- 10- 10- 4 T. The usual configuration is called a second harmonic device, which

comprises two coils formed on a common high-permeability core. An alternating current in the

excitation coil periodically saturates the magnetic core and the permeability is modulated. The

second winding is a sensing coil that couples with the excitation coil through the core. The

external measured field also affects the core's permeability and a voltage proportional to the

field strength is induced in the sensing coil at the second harmonic of the excitation frequency.

Although standard fluxgates can detect AC magnetic fields they generally have an upper limit of

- 1 kHz, although recent publications have claimed to have achieved a bandwidth of- 1 MHz.

Hall-Effect A particle of charge, q, moving with a velocity,~. in a magnetic field, !1. is subject to a Lorentz

force

(2.1)

which acts in a direction that is perpendicular to~ and fl. The Hall Effect is the influence of the

Lorentz force in a semiconductor material. A voltage applied across a block of semiconductor

material causes a current to flow. If a magnetic field is applied perpendicularly to the current,

then & will cause the charge carried to be deflected in the third dimension. This results in a

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Chapter 2

build up of charge and a potential difference is developed across the device in the direction

perpendicular to the applied voltage and measured magnetic field. Hall sensors typically use n­

type silicon for low-cost applications although other semiconductors such as InAs and AnSb can

be used where greater frequency response and sensitivity are required. This enables easy

integration with other semiconductor elements to create sensors integrated with controlling and

processing electronics.

Magneto ~resistive

The magnetoresistive effect is the property of a current-carrying ferromagnetic material to

change its resistivity in the presence of an external magnetic field. Such a material is permalloy,

which consists of 80 % nickel and 20 % iron and has a high magnetic permeability. Figure 2.2

shows the influence of an external magnetic field on the magnetisation of a strip of material

such as permalloy. The device is arranged such that when there is no external magnetic flux,

the current flows parallel to the magnetisation vector, M. On the application of an external flux,

f1, perpendicular to the current flow, M will rotate by an angle a., which changes the resistance

by

(2.2)

where R0 and L1R0 are material properties.

!l.

I ~I I

Figure 2.2. Magnetoresistive effect: a current, I, flows through a ferromagnetic material and an external magnetic flux, !l., causes the magnetisation vector, M, to shift by an angle a.

2.2 Design Requirements

To gain an insight into which magnetic sensor technologies are suitable for the task in hand,

values of the field magnitude and frequency were required. Initial investigations with a Hall

probe gaussmeter were unsuccessful; no changes from the background readings were observed

in either AC or DC modes. This was assumed to be because the gaussmeter had either too low a

sensitivity or too slow a frequency response.

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Chapter 2

The simpler idea of using a single loop of wire around the end of the sensor barrel was more

useful. The circuit was connected directly to a 20 MHz analogue oscilloscope to obtain a

smooth trace (amplitude noise less than the thickness of the trace) with a period of 10- 6 s,

which is in agreement with the manufacturer's stated operating frequency of 1 MHz. The EMF

across the loop had a sinusoidal form that varied with time, t, as

V = V0 sin (2Jift) (2.3)

where V 0 is the amplitude and f is the frequency. Faraday's law gives the relation to the

magnetic flux, r/Jm, through the loop as

with

V= -dr/Jm dt

r/Jm =BA

(2.4)

(2.5)

where B is magnetic flux density and A is the area of the loop. This leads to an expression for B

B = - ~ f V (t )dt

=-~ fsin(2Jift )dt

V: = --0 - cos(2JTft) +constant A271/

(2.6)

When the EMF is at a maximum or minimum, the field is changing at its fastest rate

(corresponding to B = 0), so there is no offset and the integration constant is zero, thus

B = B0 cos(2Jift) (2.7)

with the amplitude of the field

B=~ 0 A271/

(2.8)

With no target present the EMF across the loop was measured as 0.134 V, so using the barrel

diameter of 73.7 mm gives an estimate for the field amplitude B0 - 5 x 10- 6 T.

The coil can be modelled as a solenoid such that the flux inside the coil is constant except

near the edges where its magnitude decreases as the field lines diverge. The test loop was fitted

near the end of the sensor barrel and so an estimate of the magnitude of the current in the coil, /0,

can be estimated by the simple function

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Chapter 2

(2.9)

where f.J.o is the permeability of free space and n is the number of turns in the coil per unit length

of the coil; this assumes a one-layer thick coil. Using the estimate of B0 gives the estimate

n/0 - 10 A.turns.m -J. If the coil has, say, 1000 turns and is approximately 8 cm long, then the

current in the coil, /0 - 10- 3 A, which is a reasonable value that gives confidence in the

suitability of the B0 estimate.

2.3 MagnetoaResistive Sensor

The equation describing the rotation of the magnetisation with applied field (2.2) shows that the

magnetoresistive (MR) effect is non-linear. The effect can be linearised by depositing

aluminium stripes - so called Barber poles - on top of the permalloy at 45 a to the strip axis.

The conductivity of aluminium is larger than the permalloy and so the strips rotate the current

direction through 45 a. The current follows a zigzagged pattern which effectively changes the

angle of rotation of the magnetisation relative to the current from a to a- 45 a. For the Philips

KMZ series of MR sensors four permalloy strips are arranged as the arms of a Wheatstone

bridge arrangement. For two diagonally opposed strips the Barber poles are at + 45 a and - 45 a

to the strip axis. When an external magnetic field is applied, as the resistance increases in one

pair of strips it is matched by a decrease in resistance in the other pair. The result is a bridge

imbalance that is linearly related to the magnitude of the applied magnetic field.

Philips state that their KMZ10A thin-film permalloy MR sensor is suitable for a wide range

of applications including navigation, current and field measurement, revolution counters,

angular and linear position measurement and proximity detectors [33]. The navigation using

Earth's magnetic field (- 5 x 10- 5 T) was of interest because the estimate of B0 given in the

previous section ( § 2.2) is just an order of magnitude less (- 5 x 10- 6 T). It was anticipated that

with suitable amplification circuitry these devices could be used to measure the field. The

KMZ10A devices were selected because of their availability and the fact that they are quoted as

being capable of operating at 1 MHz.

2.3.1 Amplification Circuit

As a quick trial the MR device was tested by connecting it directly to a power supply and an

oscilloscope. This demonstrated that the device was functioning normally and a reading was

obtained when a magnetised screwdriver was placed in its vicinity. However to detect weaker

fields an amplification circuit must be used; the Philips data sheet [33] gives a basic application

circuit which was constructed on a PCB. The circuit allows for sensor offset and sensitivity

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Chapter 2

adjustment, as shown by the circuit diagram of figure 2.3. Temperature drift is an important

consideration and the circuit diagram shows the use of a compensatory silicon device with a

positive temperature coefficient (R6). However, this device cou ld not be sourced, so by plotting

the expected resistance response to temperature a suitable resistor was found to optimise the

circuit for the laboratory temperature.

r-~--~----------~----------~r---~------------~~~:5V sensitivity offset

adjustment R7 R1 R2 R5 2.4 kll

500 kll 140 kll

RB 2.4 kl.l

R9 33 kll

R11 22kll

R10 33kll

adjustment

,li>--7 +---oVa: 0.2 V to 4.8 V

Ct 10 nF

(with resistive load greaterthan 10 kll)

MBH687

Figure 2.3. Amplification circuit used with the MR sensors. Adapted from [33].

The PCB was double sided and space between tracks was left un-etched and grounded to

reduce noise levels and the resulting circuit is shown in the figure 2.4.

Figure 2.4. Constructed amplification circuit with the MR sensor protruding from the left-hand edge.

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Chapter 2

2.3.2 Circuit Testing

The circuit was tested by connecting the output to an oscilloscope and moving a magnetic field

from a screwdriver in the vicinity of the MR sensor. The result was a response at a higher

amplitude voltage level than was obtained with the circuit in the previous section (§ 2.3.1), as

would be expected. However, when the MR sensor was placed near the IDS coil, no response

was noticeable above the background noise levels. There were two possible reasons for this,

firstly the circuit may not have been sensitive enough and secondly the frequency of the IDS

coil may have been too high for the sensor to detect.

To investigate the frequency response of the MR sensor, the IDS coil was removed from the

usual oscillator/demodulator circuit and connected to a frequency generator. The lDS coil was

placed above the MR sensor, but no response was found at any frequency. At 1.00 MHz the

coil voltage was 427 m V and the influence on the field sensor as monitored on the oscilloscope

was a low-level background noise(- 1.0 MHz, - 1.26 mV). At 400kHz the coil voltage was

182 mV and there was no distinguishable effect over the background noise (- 3.4 MHz,

- 2.5 mV). The lower coil voltage is a result of a shift down from the resonance frequency of

the coil. Similar experiments using a different coil with a much lower resonance frequency of

35 kHz also failed to yield a useful signal response. It is suspected that the low voltage and

current provided by the signal generator produced a field of insufficient intensity for the MR

sensor to detect. The KMZIOA data sheet shows that the response to magnetic field decreases

as the frequency increases, so the lack of response from the circuit was likely to be a result of

the combination of low amplitude and high frequency. Hence this device was shown not to be

appropriate for this application.

2.4 Test Coil Sensor

Besides the MR sensor, the other magnetic field sensor identified in § 2.1 that fulfils the

requirements of § 2.2 is the test coil. Equations (2.3) to (2.8) can be used to determine the

amplitude Bo given a measured potential difference (V0) across the test coil. However, since the

coil consists of multiple loops, the total flux is that passing through an individual loop

multiplied by the number of turns in the coil, N. Therefore the magnetic flux density can be

determined from the measured EMF by

B = Vo o AN2Jlf

(2.10)

A simple test coil was formed by wrapping 26 gauge (0.4038 mm) enamelled copper wire in

28 turns around a plastic former of diameter 11 mm and length 10 mm. A glass capillary tube

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Chapter 2

was used as a holding support for the tube and the signal wire passed though the middle and out

the end to an oscilloscope. The coil is conducting, but it does not interfere with the operation of

the lDS since it is stranded and therefore eddy currents cannot be generated in it. However, it is

not possible to measure a physical quantity from a system without affecting the system itself. In

this situation, the coil takes energy from the field and will have some influence on the system.

copper wire

Signal wire out ~

Non-conducting holding rod

Figure 2.5. Simple test coil construction.

Placing the test coil below the lDS coil produces a clear sinusoidal signal with a I MHz

frequency. Immediately below the sensor coil the magnitude of the potential difference across

the test coil was recorded at 84 m V; corresponding to B0 = 5.0 x 10- 6 T. The values given by

the test coil are in agreement with the estimates in § 2.2.

2.5 Selection and Refinement of Test Coil

It can clearly be seen that the results from the test coil are much more stable and well defined

than from the MR sensor. Test coils are well suited to measure the AC magnetic fields

generated by the lDS coil since Faraday's law relies on changing fields to generate a potential

difference. This effectively eliminates the static background effect of Earth's magnetic field.

The test coil was used to measure the magnetic flux density profile of the lDS coil, as shown

in figure 2.6. The test coil was positioned immediately below the lDS coil and the vertical

component of the flux recorded at different displacements from the centre position. It can be

seen from this profile that, as expected, the field is strongest in the centre and decreases

outwards. At the edges of the lDS coil, the field drops by an order of magnitude and at a

displacement of 35 mm from the centre - which corresponds to the edge of the IDS coil - the

field is 36 % of the centre value. Beyond 35 mm the flux density was very small and with the

trial test coil the signal was lost in the background noise. Consequently careful design of the

test coil was required to give strong coupling to the lDS coil.

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5

r-~ 4

I 0

2

-40

Chapter 2

-20 0 20 40

x /mm

Figure 2.6. Magnetic flux density profile of the lDS coil as measured with the test coil.

2.5.1 Test Coil Construction

The test coil described in § 2.4 was refined to give a stronger signal towards the edge of the lDS

coil. The use of a core with a high permeability would increase the potential difference across

the test coil but this would interfere with the operation of the lDS since eddy currents can be

generated in the material. Another way to increase the signal is to increase the total area of the

coil by increasing the number of turns or the diameter of the core. A good coil has a large

number of evenly-spaced, tightly-wound loops.

The test coil design process went through many stages before a final refined option was

developed. Test coil 'a' shown in figure 2.7 was constructed using 32 gauge (0.2032 mm)

enamelled copper wire with an air core and was held together with wire braces. It was found

that the wire braces produced spikes on the signal and so coil 'b' was constructed in a similar

way, but was held together with masking tape. For both of these designs the intention was for a

flat sensor, so that only the vertical component of the field was detected. Their actual height

was - 2 mm, which limited the number of turns to - 40 and so a strong signal could not be

obtained. More turns were introduced in test coils 'c' and 'd' which had lengths of- 6 mm and

were constructed on paper formers. These test coils had approximately 80 turns and produced

clear signals with improved amplitude. Coil 'e' demonstrated the use of finer 40 gauge (0.0787

mm) wire enabling a higher turn density.

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Chapter 2

I l

1 '

I

(b) liHfl(lllffilllllll cc) ~ IIII)Uilllllljllll]ll (d) Jllllill~illllffi (e) am1mnm 1 tfo th 112 I 1 3 14 titS ita ili ' 1!8 ili

Figure 2.7. Different coil designs.

During the development of test coils 'a'-'d' marked improvements in signal to noise ratios

and sensitivity were recorded, however these coils were flimsy and were not suitable for making

a large number of measurements. The final test coi l 'e' in figure 2.7 was a much improved

design that uti lised a non-conducting solid core and two end pieces to hold the wire in place; the

construction is shown in figure 2.8. The test coil had 200 turns which gave a voltage of 240 m V

at the centre of the IDS coil.

, .. 11 mm "I

}mm , ..

9mm

"' (a) (b)

Figure 2.8. Optimised test coil design. (a) Side view. (b) Projection view.

2.5.2 Test Coil Characterisation

The impedance of the test coil was measured using an Agilent 40Hz - 110 MHz impedance

analyser. This device sweeps through a range of frequencies to determine impedance as a

function of frequency , as shown in figure 2.9. The peak in impedance magnitude of 113 ill is

at 1.38 MHz, which also corresponds to the point where the impedance phase changes from

+ 90 o to- 90 °. Note that this is a peak in the complex magnitude of the impedance and does

not correspond to a re istive peak.

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"' "' ~ 00

" "0 -Q::,

Chapter 2

100 150 ·-·----··--·-·-·-··------······----··--·

50 c: 100

0 -"

~ 50 -50

- lOO

0.1 10 0.1 10

f I Hz f I MHz

(a) (b)

Figure 2.9. Impedance analysis of the test coil. (a) Impedance phase angle 0. (b) Impedance magnitude IZI.

The form of figure 2.9 indicates that the coil is a parallel R, L and C circuit as shown in figure

2.10 and the peak corresponds to parallel R, L and C resonance. The resistance, R, results from

the length of wire, the coi l loops result in an impedance, L, and the capacitance, C, is the

consequence of charge building between loops. The impedance of the coil, Z, can be regarded

as the opposition to current flow, I , such that the potential difference across the inductor is

V= I Z . The inductive element of the coil impedance is X L= iwL , where i = ~, w is the

angular frequency of I and L is the inductance. The capacitive element of the impedance is

X c = 1/iuC , where C is the capacitance. The admittance, Y, is defined as the reciprocal of

impedance, i.e. Y = 1/Z, and for the parallel LR and C circuit is given by

1 Y= +iwC

R + iwL (2 .11 )

In polar form, Y = IYicp, this is

(2.12)

At resonance the phase angle, cp, is zero and equation (2. 12) shows that thi s is when

(2.13)

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Chapter 2

and thus the resonant frequency is

(2.14)

At resonance when the phase angle is zero, the impedance is entirely real and thus from

equation (2.11) and using equation (2.13)

Y= R = R R 2 + mr/ L2 L/C

Z=~ (2.15)

RC

The AC resistance is much higher than the DC resistance because of the skin and proximity

effects. Passing a direct current through the test coil reveals that R = 13.3 n. Substituting this

value and the resonance data from figure 2.9 into equation (2.15) gives a values of

L = ~ ~ZR- R 2 = 8.8 X 10- 4 Hand c =L/ RZ = 5.9 X w-IO F.

c

Figure 2.10. Parallel R, L and C circuit model of test coil.

2.6 Collection of Data

With the test coil designs completed, it was then appropriate to test the collection of data. Initial

tests revealed low level noisy signals and efforts were made to improve them using a phase­

locking technique.

2.6.1 Signal Noise

The test coils were connected to an Agilent 500 MHz 2 GSa.s- 1 digital oscilloscope and the

traces were recorded. The recorded signals were found to be subject to noise and fluctuations

39

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Chapter 2

that made them difficult to use. Figure 2. 11 (a) demonstrates the fluctuations over 200 cycles

with a sample rate of 100 MSa.s - 1 and it is clear that there is not a smooth signal as the

amplitudes vary from 2.5x 10 - 3 -7.5x 10 - 3 V. Figure 2.11 (b) shows high frequency noise on

the signal over 10 cycles.

l.E-02

5.E-03 5.E-03 > -g O.E+OO -;;; O.E+OO " bJl en

-S.E-03

- l .E-02 -+-----.-----,---,.------j

O.OE+OO 5.0E-05 l.OE-04 1.5E-04 2.0E-04

t I s

(a)

bJl

en -S.E-03

- l .E-02 -+----.---.---,.-----.-~------"

O.E+OO 2.E-06 4.E-06 6.E-06 8.E-06 l.E-05 I Is

(b)

Figure 2.11. Signal recorded from a test coil. (a) Global varia tions. (b) Local variations.

To clean up the signal, the digital oscilloscope includes an averaging fac ility that takes the

mean of repeating functions. However this was not used because it was expected that in

practical use, the amplitude of the field would vary over time and this information would be lost

in the average. So a phase- locki ng technique was employed, which relies on knowing the basic

form of the signal that is being measured. The noisy time-dependant input signal g (t) is

compared to a known smooth time-dependant reference signal f(t) by means of a general

correlation funct ion

R(o)= Lim- J(t) g(t+o)dt 1 {r t ->~ T

(2.16)

which relates f and g for a time parameter c5 and where T is just the upper integration li mi t. R is

zero when f (t) and g (t) are independent. Generall y g (t) is modulated in some way by the

referencef(t) . In the case of the IDS the signals are known to be periodic sine functions with

ampl itudes a , and a2 and of frequency cv, thus the correlation function becomes

a a f, "T R(nT, r/J ) = - 1-

2 sin(wt )sin(UJt + rp )dt nT o

a a =-1 -

2 cos rp 2

(2.17)

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Chapter 2

which has an upper integration limit of nT where T is the period of the frequency w and n is an

integer. rp is the phase difference betweenf(t) and g (t). For complete correlation R is taken as

unity and if the amplitude of f(t) and the phase difference are known, the amplitude of the

signal may be determined. This technique is appropriate to the test coil signal because the

signals are small, periodic and noisy.

Lock-in amplifiers apply phase-locking and can be used to reduce the noise on a signal where

there is a clear reference. A lock-in amplifier was tested and a smooth reference signal was

taken from several loops of wire wrapped round the IDS barrel. However it was found that this

instrument was not suitable for the high frequency signal from the IDS and on further

investigation revealed that I MHz devices are uncommon.

2.6.2 Phase-Locking Program

Given the inability of the hardware lock-in amplifier to resolve the signal, an offline software

solution was investigated. The digital oscilloscope was able to record actual values from the

signal which enabled the development of a Java application to phase-lock the recorded signal.

The signals were stored as text in comma separated value (CSV) formatted files. The program

extracted data from a specified file and proceeded to multiply the signal and reference together.

The product was then integrated and the resulting amplitudes plotted on the graphical user

interface (GUD. The phase difference between the signal and reference was adjusted by moving

a sliding bar and both an average amplitude and amplitude variance were calculated. Figure

2.12 shows a screenshot from the program. An optimisation method was developed to find the

phase that gave the minimum amplitude variance i.e. the smoothest output signal. The resulting

amplitudes array could then be saved to a file in CSV format to enable display in a graphing or

statistical package.

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Chapter 2

.. . l:...li;ll.l!1

~ -- ~-- =~ ~· ...... p; ... ... __

{:0 t•t4038108736C893

' ,_. --- .~ 1 I '~ I Pl12 PI 4AI3 -

Figure 2.12. Screen-shot from the phase-lock Java application.

Figure 2.13 shows the result of phase-locking a noise signal with the program. Although it

may appear irregular, it is smoother than the unprocessed signal. The average amplitude is of

the unprocessed signal is 4.65 x 10 - 4 V with a variance of 4.39 x 10 - 7 V2. The phase-locked

signal has a mean amplitude of 0.0324 V with a variance of 1.12 x 10 -? V2•

> .._ .g 0.033 .@ 0.. ~ ~ 0.032

iZi

0.031 +-----------,,-----,-------1

O.OE+OO S.OE-05 l.OE-04

t I s

l.SE-04 2.0E-04

Figure 2.13. Result of phase-locking an input signal.

For practical purposes a second application was developed without the GUI to process the

recorded signals in bulk. A list of input signal and reference fi les were given to the program

that then opened the fi les, found the optimum phase difference and saved the resulting

42

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Chapter 2

amplitudes to an appropriate CSV file. With this program a set of readings from a whole

experiment could be processed in one batch.

2.7 Summary

This chapter has described a number of magnetic field sensing technologies and has discussed

their relative merits and suitability for measuring the field around an lDS coil. An initial

investigation showed that the field oscillated in a sinusoidal manner with an amplitude of

- 5 x 10- 6 T and a frequency of I MHz. Magneto-resistive sensors and test coils were selected

as being the most suitable devices to measure fields of this form. Initial investigations of a

Phi lips KMZIOA M-R sensor were unsuccessful and this was attributed to a combination of the

high frequency and low strength of the field. Trials of a test coil device were more fruitful and,

after a number of refinements, a suitable coil was constructed. The signal from the test coil was

found to be very clean at high field strengths, but for low field strengths ( < 2 x 10- 6 T) the low

signal to noise ratio was found to be a serious issue. To address this problem, the signal was

recorded with a digital oscilloscope and then a phase-locking program was built to extract the

amplitudes from the noisy pattern. Before processing, an example signal was found to have a

mean amplitude of 4.65 x 10- 4 V with a variance of 4.36 x 10- 7 V2, but the phase-locking

technique revealed an amplitude of0.0324 V with a variance of 1.12 x 10- 7 V2• The result was

a reliable system that could be used to measure the magnetic field around IDSs.

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Chapter 3

Finite Element Analysis

In the first chapter it was hypothesised that small magnetic field changes that are not detected by

coil impedance measurements can provide more information about the target material. The

previous chapter described the development of a sensor that was suitable for measuring the

small fields around IDS coils. This chapter leads on from this by describing how finite element

analysis (FEA) was used to determine what field features can offer useful additional information.

Firstly there is a description of the electromagnetic finite element modelling processes and how

it was applied to the IDS coil and target arrangement. Both two- and three-dimensional models

were constructed using a commercial software package and there is a discussion of the relative

merits and applications of each. The models provided a large number of data, so a convolution

program was developed to take the magnetic field solutions and extract measurements of a

similar form to those taken by the test coil experiments.

3.1 Generalised FEA Modelling Process

Analytical solutions to eddy current problems are described by Dodd and Deeds [34] who give a

quick and easy method for the calculation of observed effects. However, the solutions presented

there are not appropriate for high frequencies. This is because as the frequency of current in a

wire increases, the current density ceases to be uniformly distributed and tends to concentrate at

the surface, which causes the coil resistance to increase and the inductance to decrease. This

leads to an effect where the current tends to flow across the turns rather than through them and

the capacitance between the coil and target increases. So given that an analytical solution is not

available, numerical approximations are needed.

In general terms the finite element method is used for the solution of physical problems that

are described by differential equations. The continuous domains of the problem are broken

down into a finite number of elements. Chari and Silvester [35] and Silvester and Ferrari [36]

describe the finite element method with particular reference to electrical and magnetic field

problems.

There are a number of commercially available software suites that enable FEA of

electromagnetic problems. Simulations for this thesis have used Ansoft's Maxwell software

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Chapter 3

suite, which consisted of two main programs that could be used to solve problems in two- or

three-dimensions. The programs used FEA to numerically solve Maxwell's equations over a

specified geometry and within user-defined boundary conditions. All simulations were

completed on the same 2.2 GHz, 5 I 2MB RAM PC with the Microsoft Windows XP (service

pack one) operating system. Therefore it was possible to use the time taken to complete the

FEA to compare the efficiency of various methods.

3.1.1 Setting Up the Simulation

The first stage of the modelling process is to construct the problem geometry to give the

program the physical constraints within which the solution is to be found. Then the material

properties such as the relative permeability, J1, relative permittivity, £, and conductivity, a, are

entered; this may be done manually or common materials can be selected from a predefined

catalogue. Following from that, sources and boundary conditions are entered, which define the

problem to be solved. One or more of several so-called executive parameters may be selected,

which are quantities such as force, torque, inductance, capacitance, or power loss. These

parameters may arise as a result of fields generated by the sources and can be determined by the

program. The program will then proceed to solve the problem through using a FEA method by

generating a mesh and calculating the field solutions. Results can be extracted through the use

of a post processor program that uses the field solutions to determine various properties such as

magnetic field strength.

3.1.2 Impedance Simulation

The Maxwell software allows for the calculation of an impedance matrix, which summarises the

relationship between AC voltages and currents in multi-conductor systems. For a two­

conductor system, the equivalent circuit is shown in figure 3.1, which is a generalised form of

that given in figure 1.3.

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Loop 1 (IDS coil)

Loop 2 (target)

Figure 3.1. Equivalent circuit for a two-conductor system.

The potential difference across each loop are given by

This leads to the matrix expression

Chapter 3

(3.1)

(3.2)

(3.3)

where Z1 = R1 + iwL1 is the impedance of loop one, Z2 = R2- iwL2 is the impedance of loop two

and ZM = RM + iwLM is the mutual impedance between loops one and two. For a system with 11

conductors, the impedance matrix contains 11 x n elements. Once the field solver has completed,

the impedance solver can use the field values to calculate the inductance and resistance values

separately before combing them into the impedance matrix.

The inductance is calculated from the average energy of the system, U , which is given by the

integral of the magnetic field density, f1, and magnetic field, H, over the volume, V, of the

problem, thus

U =.!_ fB·H* dV 4--v

At any point in the current cycle, the energy of the system, U, is given by

(3.4)

(3.5)

where L is the inductance and I is the current at a given in time. Integrating over the current

cycle, gives a second expression for U

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Chapter 3

(3.6)

where IRMS is the root-mean-square current and fpeak is the peak of the current cycle. Thus the

inductance can be determined from

lll·H*dv L=----:::-­

I~eak (3.7)

The Maxwell program takes /peak = 1 A. turn- 1 and so a value for the inductance can be

calculated.

The resistance is calculated from the power that it dissipates, which is given by the integral of

the current density,!._, over the volume of the problem, thus

P = -1- fl · J* dV 2 --av

A second expression for the power is

2 1 2 p = R / RMS = l R J peak

Thus the resistance can be determined from

Coil Impedance Estimate

~ lLL*dv R=--,--­

I~eak

(3.8)

(3.9)

(3.10)

To compare the result of the simulations with the actual coil values, an estimate of the coil

impedance was found using some of the estimates from section § 2.2. The resistance of the coil

can be estimated by treating the coil as a hollow copper cylinder with a thickness of 1 mm, a

height of 75 mm and a diameter of 70 mm. This gives a value of R- 5 x 10- 5 n. The

inductance can be estimated by treating the coil as a solenoid with an air core such that

(3 .11)

where N is the number of turns in the coil, A is the coil area and l is the coil length. This yields

a value of L - 10- 3 H for a 1 00-turn coil and L - 10 -? H for a single-turn coil.

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Chapter 3

3.1.3 Eddy Current Solver

The eddy current field solver is used to simulate the influence of time-varying magnetic fields

on conductors. All time-varying fields, £(t), are assumed to be sinusoidal and oscillating at the

same frequency, w, and phase, B, with the form

(3.12)

where F0 is the field amplitude. All fields must have the same frequency, but do not have to be

in phase. Problems involving non-sinusoidal fields must be broken into harmonics and solved

at each frequency. For the IDS coil and target system the magnetic field measurements

described in section § 2.2 show that the field is of the form of equation (eq 3.12).

Maxwell's equations for the fields in the problem are

oB VxE=---= - of

V-B=O

oE Vxfl=fLl+fLE

0--;

(3.13)

(3.14)

(3.15)

(3.16)

where §;_ is the electric field, !1 is the magnetic flux intensity, p is the charge density, E: is the

permittivity, f1 is the permeability and .f. is the current density. There are also a number of

relations: magnetic flux intensity and magnetic field, !1 = JlH; electric flux and electric field,

D = cf;.; and current density and electric field, .f.= crf;_, where fJ is the conductivity. Fields in the

form of equation (3 .12) can be expressed as

and therefore

and

F(f) = Re[F0 exp(iB)exp(imt )]

ofl. =iwB of

of;_ =iwE or

Thus Maxwell's equations (3.14) and (3.16) for a time harmonic field can be expressed as

(3.17)

(3.18)

(3.19)

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Chapter 3

VxE=-iwB - - (3.20)

V x.lB = aE + iwEE Jl- - -

(3.21)

Let a vector potential, A, be defined with the equation

B=VxA - - (3.22)

Equation (3.22) may be substituted into equation (3.21) to give

V x-}(V xA) = afi + iwcfi (3.1)

As described by Weiss and Csendes [37] a solution for !1.. in terms of A and qJ is given by

!1.. = -iwA- V rp (3.23)

where qJ is a scalar potential function. Substituting this into (3.22) yields

(3.24)

The right-hand side of this equation is of the form of a complex current density with the three

components. The electric potential results in a source current density

Js =-aVrp (3.25)

Time-varying magnetic fields result in an eddy current density

(3.26)

The remainder is the result of time-varying electric fields and can be described as a

displacement current density

(3.27)

The sum of equations (3.25), (3.26) and (3.27) is the total current density, Jr. When modelling

conductors connected to an external source, the total current in the conductor, fr, must be

specified and thus lr is specified by the integral over the cross-section of the conductor Q

(3.28)

The eddy current solver calculates eddy currents by solving for A and qJ in equation (3.24) and

utilising equation (3.28).

The eddy current solver cannot use these equations for non-linear materials because although

the current is sinusoidal, the fields associated with non-linear materials consist of a number of

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Chapter 3

harmonics. Ansoft's Maxwell programs utilise an effective magnetic flux density and effective

magnetic field intensity, which depend on the frequency of the harmonics. This is described in

more detail in the Ansoft technical manual [38].

3.ll.4 Solution Criteria and Meshing

The FEA solver breaks the problem space into a mesh of smaller elements over which the

program can solve the differential equations. In general, the elements may be any shape, but in

the Maxwell program triangles and tetrahedrons are used for two- and three-dimensional

problems respectively. A number of options are available to produce a solution with the desired

accuracy. The meshing process can be wholly automatic, wholly manual, or a combination of

both.

The entirely automatic process generates an initial coarse mesh that is refined over a number

of passes. After each pass, a value of the error in the field is calculated and the mesh is refined

by a specified amount to reduce this error for the next pass. Once a user-specified target error

has been reached, the solution process will stop. To put an upper limit on the maximum time

that the solver will attempt to meet this target, the user may also specify the maximum number

of passes that are to be completed before the process will stop regardless of the error. The result

is a finer mesh around material boundaries and in the corners of objects.

The manual meshing process allows the user define smaller elements in specific areas of

interest; that particular mesh is then solved on an as-is basis. The final meshing method

involves a combination of both manual and automatic processes; the meshing program is given

a direction with a manual initial mesh and then the automatic refinement process is applied.

The solution process for finer meshes is more computationally intensive and requires more

memory than coarser meshes. So the desired accuracy must take account of the available

resources. For example, with the IDS and target arrangement, the area between the coil and the

target is of particular interest and so the space in this region can be refined while the remainder

of the problem can be left with a relatively coarse mesh. The result is that the error in the field

between the coil and the target is lower than other areas that are not of particular interest.

The meshing process can be controlled by specifying mesh properties for individual objects,

which can be done by either setting the maximum element size or the maximum number of

elements. This can be exploited by using dummy objects that have no electrical properties, and

no function in the problem, but have tighter mesh properties than the surrounding areas. For

example, the region between the IDS coil and target can include a dummy object with a much

finer mesh than the surrounding region and so more accurate field solutions will be found in that

particular area of interest.

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Chapter 3

Within each solver pass there is also an iterative process to refine the field solution; the

maximum number of iterations can be specified before the solver is started. A normalised error

quantity called the solver residual is used to specify acceptable tolerances for the solution; for

linear materials there is a linear residual and for non-linear materials there is a non-linear

residual. A residual is calculated after each iteration: if it is higher than the specified value a

correction is added and another iteration is completed, if it is lower than the specified value then

no further iterations are run.

The Maxwell program can produce solutions through one of two methods. The first is a

direct method that will always converge to a solution and the second is a more intelligent

method that is generally faster for problems with large meshes, but does not always converge.

The decision as to which method is used can be left to the program by selecting the automatic

mode that makes an estimate of whether the faster method will work. If the estimate is incorrect

and the faster method does not appear to be converging, then the process is stopped and the

direct method is used.

3.2 TwoaDimeJrnsJional IFEA

Ansoft's Maxwell 2D Field Simulator uses FEA to numerically solve two-dimensional

electromagnetic problems. A problem is entered into the program and field solutions are

calculated as described above. Two-dimensional simulations are appropriate to schemes such as

the IDS coil with a target centrally positioned below it.

3.2.1 Test Problem

A basic model of the IDS sensor coil and target arrangement was used to investigate the

effectiveness of the two-dimensional FEA.

Geometry

One of two coordinate systems may be utilised for drawing the geometry of a two-dimensional

problem. The first is an xy-plane Cartesian coordinate system, which is appropriate for any

cross-sectional geometry. In this system, the current flows in the z-direction and therefore the

magnetic field lies entirely in the .xy-plane with no z-component. The second is an rz-plane

cylindrical coordinate system, which is suitable for axial-symmetric problems. In this system,

current flows in the 8-direction around the device's axis of rotational symmetry and therefore

the flux only has components in the rz-plane. The problem geometry of the IDS sensor coil

with a centred target can utilise the latter scheme, as shown in figure 3.2. It should be noted that

using this coordinate scheme means that the target is modelled as disc rather than a rectangle.

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Chapter 3

The assumptions about the geometry of the coil were taken from a discussion with the UK

supplier of the IDS and from the Kaman user manual [ 1 0]. The coil is taken as being a 1 mm

thick cylinder with an external diameter 1 mm less than the outer carbon fibre protective casing.

The target was taken as being a 5 mm thick rectangular plate positioned at d, = 10 mm, with a

width 3 times the coil diameter to avoid problems associated with small targets (§ 1.4.2).

lDS coil cross­

section

' Vl I '< I 3 : 3 1(1) 1:::;' I '<

35

~ I 79

/

Target

d,

:~O!!l~~~~~~~~·:fs I )08 I I I

r

Figure 3.2. The axial-symmetric geometry of the lDS sensor coil and centred target. Dimensions given in mm.

Materials The IDS coil was assumed to be a copper construction and therefore appropriate material

parameters were selected: t:,. = 1.0000000, p,. = 0.9999910, a= 5.8000000 x 10- 7 S.m- 1. For

the purposes of the simulation the target was taken to be aluminium with t:,. = 1.000000,

p,. = 1.0000210, a= 3.800000 x 10- 7 S.m -I. The remainder of the problem space was set to be

a vacuum (c,. = 1.0000000, Jlr = 1.0000000, a= 0.0000000 S.m- \ which is a good

approximation to air (c,. = 1.0006000, p,. = 1.0000004, a= 0.0000000 S.m- 1) and was expected

to result in a faster solution.

Boundaries The IDS coil consisted of wound copper wire and so eddy currents could not develop in it,

therefore in the simulation it was set to be "stranded". The aluminium target, however, did

experience eddy currents on the surface as a result of the excitation from the coil, therefore the

default Neumann eddy current boundary was applied. Using the estimate of the coil current in

section § 2.2, the current density in the coil was estimated to have a magnitude, 10 = 10 4 A. m- 2

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Chapter 3

over the whole cross-section. The outer balloon boundary that contains the whole problem was

set to pad all the problem geometry by 200 %.

Solution

The impedance matrix was set to involve the coil and the target material. The solution criteria

were set so that the solver used the automatic mesh process with 15 % refinement per pass to

solve for both the field and the impedance matrix with a residual of 10 - 5. The solver was then

set to find a solution with a maximum error of 1 %, which took approximately 30 seconds on

the computer specified in section § 3.1.

Results The impedance matrix yielded a coil resistance of 1.617 x 10- 4 n and an inductance of

4.051 x 10 - 8 H. The inductance value is the result for a single-turn coi l and so there is

agreement to within an order of magnitude with the estimate of coi l impedance found in section

§ 3.1.2.

A plot of the magnetic field calculated by the simulation is shown in figure 3.3. This shows

that the FEA has produced field results that instinctively make sense in terms of a simple

representation of the problem i.e. the field is strongest around the coil and decays with

increasing distance from it and the field is compressed by the target and the eddy currents

generated in it. The edge of the target affects the field such that it appears to bulge at this point,

which is discussed in section § 3.4.2.

lDS coil cross-section

Target

> I0 - 5 T

I0 -6 T

I0 - 7T

< IO - s T

Figure 3.3. The magnetic flux plotted for the two-dimensional test problem. The central lighter portions represent a stronger field than the surrounding darker regions.

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Chapter 3

A plot of the magnitude of the z-component of the field taken along a line parallel to the

target, but 1 mm below the base of the lDS coil, is given in figure 3.4. On this plot radius

R = 0 mm is the left-hand edge of the problem space, which is the centre of symmetry and lies

below the centre of the lDS coil. It is the magnitude of the z-component that is of interest, since

this is the quantity that is measured by the test coil system described in section § 2.5.2. The plot

reveals local discontinuities which result from areas of the mesh that were not well refined.

Recall that the external radius of the simulated lDS coil was 36 mm and this corresponds to the

point on the figure where the plot drops to zero. This zero figure means that the field no longer

has a z-component and - recalling that the field cannot have a B-component - must therefore

only have an R-component. Investigation of the phase revealed that the field flips direction at

this point, which instinctively makes sense in terms of a simple representation of what is

happening to the field from the coil: at a given point in the coil's current cycle the field lines

extend downwards from the centre of the coil (strong vertical component); below the edge of

the coil the field lines are horizontal (weak vertical component); and outside the edge of the coil

the field lines loop upwards to the top of the coil (strong vertical component).

4

3 f-

"' I 0 2

et)'

0 50 100 Rlmm

150 200

Figure 3.4. Variation in the magnitude of the z-component of the field, !Bzl/ tesla, with radius, R I mm, along a line 1 mm below the lDS coil.

The form of figure 3.4 is in agreement with the field measurements shown in figure 2.6 and

the magnitude of the field below the central portion of the lDS coil also agrees approximately

with the measured value of- Sx 10- 6 T.

3.2.2 Simulation Refinement

The test problem simulation produced good results that appeared to reliably represent the form

of the experimentally measured field. The error for the test problem was set at 1 % but the

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Chapter 3

discontinuities found in figure 3.4 demonstrated that this value did not correspond to the actual

error in the field solution. The meshing process required more refinement to produce a more

accurate field solution and smoother plots that could reveal more detailed information.

Therefore a dummy object ( § 3 .1.4) was introduced to decrease the mesh size in the region of

interest i.e. the space between the coil and the target.

35

IDScoil ~ cross- ~ ----._

section : 79

Dummy meshing object

Target

r

Figure 3.5. Axial-symmetric geometry of the IDS sensor coil and centred target with the inclusion of a dummy object to improve meshing. Dimensions given in mm.

Figure 3.5 shows the addition of the dummy object to the test problem geometry. The object

is simply a vacuum region within which the mesh is set to have a low initial element size. The

maximum element area in the dummy object was set to 0.5 mm2• Figure 3.6 compares the mesh

without (3.6(a)) and with (3.6(b)) the dummy object. It can clearly be seen that there are more

elements in the area of interest in the mesh with the dummy object.

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Chapter 3

(a) (b)

Figure 3.6. Mesh in the space between the coil and target. (a) The original problem without a dummy object. (b) The problem with a refined mesh inside the dummy object.

The fi eld solution took about the same time as the original problem (- 30 s) and the results

are demonstrated by the plot in figure 3.7. Comparing this graph with figure 3.4 shows that the

addition of the dummy object has successfully improved the continuity of the solution in the

region between the IDS coil and the target, without a noticeable increase in the solver time.

4

3 f-

"' I 0 2

cci' I -

0 0 50 100 !50 200

Rlmm

Figure 3. 7. Magnitude of the z-component of the field , IB,I I testa, with radius, R I mm, along a line 1 mm below the IDS coil, for a geometry with a meshing dummy object.

3.2.3 Parametric Test Problem

Using the basic model of the test coil and target, a parametric prob lem was constructed to

demonstrate the influence of different target displacements on the field . This was achieved by

setting a constraint, dr. from the base of the coil to the top of the target that was swept in five

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Chapter 3

steps over the range d1 = 0, 5, ... , 25 mm. The whole solution took approximately 2.5 min,

which is what would be expected given that one solution took 30 s.

The impedance matrix was calculated for each step and the variation of inductance with d1 is

given in figure 3.8. As d1 increases, the mutual inductance, M, between the coil and target

decreases as the coupling between the two systems decreases. Equation (1.8) shows that a

decrease in M corresponds to a decrease in the coil's equivalent resistance. Conversely,

equation ( 1.9) shows that the decrease in M leads to an increase in coil's equivalent inductance.

This theoretical analysis is mirrored by the simulation results. A further simulation, with

d, = 50 mm, showed that the curve tended to 4.36x 10- 8 H as the target's influence decreased.

";' 4.2 0

X

::t

-.J 4

5 10 15 20 25

Figure 3.8. The variation of coil inductance, L, with target displacement, d1•

3.3 Three~Dimensional FEA

Ansoft's Maxwell 3D Field Simulator uses PEA to numerically solve three-dimensional

electromagnetic problems. Like its two-dimensional cousin, a problem is entered into the

program and field solutions are calculated as described in section § 3.1. Three-dimensional

simulations are appropriate to schemes such as the lDS coil with a target not aligned centrally

so that there is no axial symmetry.

3.3.1 Test Problem

A simple model of an lDS coil with an offset target was constructed to test the effectiveness of

the three-dimensional PEA. The two-dimensional xy-plane model of the cross-section of the

problem geometry is not appropriate since it would assume that the target extended infinitely in

the z-direction and could not simulate the cylindrical coil.

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Chapter 3

Geometry

As in section § 3.2.1, assumptions about the coil dimensions were taken from a discussion with

the IDS supplier and from the Kaman user manual [10]. The problem geometry is shown in

figure 3.9. The 5 mm thick aluminium target was positioned at d, = 10 mm, had a width 3 times

the IDS coil diameter and was offset from the central position by 0.5 times the coil diameter.

An additional plane was included in the cross-section of the coil to act as a current source. The

outer boundary of the problem space was set to pad all objects by 200 %.

IDS coil --....__ 141 70l ~11 0111 1 cross-section --.........

I

79

Target offset

/ position d, /

t•, .. ~~~~~~~~ 79 o,

y

Target centred position

Figure 3.9. Three-dimensional geometry of the lDS coil and non-centred target yz-plane cross­section. Dimensions given in mm.

Materials

The appropriate materials were selected from the materials catalogue: copper coil

(£, = 1.0000000, ,llr = 0.9999910, a= 5.8000000 X w-7 S.m- 1); aluminium target

(t:,= 1.000000, fl,= 1.0000210, a= 3.800000 x 10- 7 S.m- 1); and vacuum for the remainder of

the problem space(£,= 1.0000000, ,llr = 1.0000000, a= 0.0000000 S.m- 1).

Boundaries

The IDS coil was set to be stranded to prevent eddy currents from forming in it and the current

density estimate from section 2.2 was used to set the total coil current to 0.8 A. This was the

only source in the problem and so the phase was set to zero. The eddy current effect was turned

on in the target and off in the coil.

Solution

The impedance matrix for the three-dimensional solver works in a different way to its two-

dimensional cousin and only objects with external sources can be included in the impedance

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Chapter 3

matrix; therefore the target was not included, but the coil was. The solution criteria were set so

that the solver used the automatic meshing process with the program's default values of 30%

refinement per pass with a residual of 10- 8• The solver was then set to find a solution with a

maximum error of I %, which took approximately 3 rnin on the computer specified in section

§ 3.1.

Results The impedance of the coil as given by the simulation was found to consist of a resistance of

5.36Ix 10- 5 Q and an inductance of 4.254x 10- 8 H. The inductance value is for a single turn

coil and so these values are in agreement with the estimates found in section § 3 .I .2.

Figure 3.10 shows a plot of the direction of the magnetic field calculated by the simulation.

The vectors show a snap-shot of the field at the start of the current cycle in the coil, which

corresponds to a peak in the field magnitude. On the left-hand side of the coil, the field behaves

in a similar manner to that in figure 3.3 where the field lines appear to be 'compressed' by the

target. To the right-hand side of the target the field behaves differently and there is interaction

with the target where the field appears to curl up at the edge of the target.

./

\ I /

\ I /

Figure 3.10. Magnetic flux direction plotted in the yz-plane of the three-dimensional test problem.

A plot of the magnitude of the z-component of the field taken along a line parallel to the

target, but I mm below the base of the IDS coil, is given in figure 3.Il. On this plot, the

y = 0 mm position corresponds to the point below the centre of the IDS coil. This graph has

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Chapter 3

some of the same characteristics displayed in the two-dimensional simulation results (figure

3.4): below the edge of the coiiiBzl drops towards zero and outer 'wings' tail off with increasing

distance from the centre. The discontinuities in the plot reveal areas of the mesh that are coarse

and have not produced a smooth field.

4

"' I 0

o+----===~1---------.-------~~-===~~

-200 -100 0 100 200

y /nun

Figure 3.11. Variation in the magnitude of the z-component of the field, IBzl I tesla, with position y I mm, along a line 1 mm below the lDS coil.

The form of figure 3.11 is generally in agreement with the field measurements shown in

figure 2.6, although the central portion below the lDS coil is quite different. This region

consists of two spikes below the edges of the coil and a central dip, which was not observed

experimentally. However, the magnitude of the field roughly agrees with the measured value of

- Sx I 0- 6 T; although the simulation value is slightly lower than the experimental reading.

3.3.2 Simulation refinement

The three-dimensional FEA produced a reliable simulation of the offset lDS coil and target

system. However, the rough nature of figure 3.11 showed that the mesh needed to be refined in

the region between the coil and the target. This is the same effect that was observed with the

two-dimensional simulation where the error for the test problem was also set at 1 %, so it was

thought unlikely that setting this to a tighter tolerance would yield more accurate results.

Therefore a dummy object (§ 3.1.4) was introduced to decrease the mesh size in the region of

interest i.e. the space between the coil and the target. The object was set to be a vacuum to

match the surrounding area, but with a tighter mesh to improve the field solutions. The line

from which the field profile measurements were taken lies 1 mm below the base of the lDS coil

and the dummy meshing space was constructed to include the line with a padding of 2 mm. The

maximum element size in this region was set to 0.5 mm.

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The field solution took approximately 90 min to produce a solution to the desired accuracy i.e.

30 times longer than the problem without the additional meshing space. The field profile is

shown in figure 3.12 and comparing it to figure 3.11 demonstrates that the addition of the

dummy meshing object improved the field simulation continuity albeit with a substantial

increase in solution time.

E-"' I 0

2

0+------===T---------,-----~~~-=----~

-200 -lOO 0

"/mm

100 200

Figure 3.12. Variation in the magnitude of the z-component of the field, IBzl I tesla, with position y I mm, along a line 1 mm below the lDS coil, for a geometry with a meshing dummy object.

3.3.3 Parametric Problems

The three-dimensional field simulator did not include the parametric unit that the two­

dimensional version did. However, it was possible to use a combination of operating system

batch files and program macros. For example a batch file could include instructions to start the

Maxwell program and execute a macro to construct the problem geometry, set up the materials

and boundaries and solve the problem. Once the program had finished, the next line in the

batch file was executed and a macro containing a different problem geometry could be executed.

General Macro A general macro was developed for use in the later experiments. The macro took the target

distance, d~o target width, W~o and target offset, o, in millimetres from the project file name, as

shown in table 3.1. The format of the geometric parameters was strict, although the final date

tag could be any length to include information about the project date, author, etc. Other

dimensions for the problem geometry were assumed to be constant and were set within the

macro. Using this method the batch file could run a set of problem geometries with differing

problem geometries.

61

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Table 3.1. Parameters taken by macro from project file name, where d1 =target distance, W1 =target width, Os= target offset.

General format Example

dr AAAA 0010

BBBB 0222

cc cc 0037

Date or Other Notes DD-MM-YY 01-01-00

Chapter 3

For problems that required dummy meshing objects, a macro was constructed to set the

maximum element size in the problem objects. However, a bug in the Maxwell program meant

that it was not able to utilise macros automatically for the meshing process and a work-around

method had to be used. A batch file called the general macro to construct and set up each

problem. Each problem was then opened individually and the meshing macro manually started.

A second batch file was then used to solve the problems automatically in succession.

Test Problem A parametric test problem was constructed to test the macros and investigate the influence of

target displacement on the impedance of the coil. The general macro and the meshing work­

around described above were used. The test problem geometry from section § 3.3.1 was used

with w1 = 222 mm and Os= 37 mm, but the target distance was swept in the range dr = 0, 5, ... ,

25 mm. The mesh was refined such that maximum length of elements in the target and the

measuring gap was 7.5 mm. The whole solution took 450 min, which was approximately 5

times the length of an individual problem, as expected.

The results of the simulation are plotted in figure 3.13 and show the effect described in

equation (1.7) whereby the coil inductance decreases with increasing d1• A further simulation,

with d1 = 50 mm, revealed that the inductance tended to 4.58x 10- 8 H as the influence of the

target decreased. This value differed slightly from the two-dimensional result

(L--+ 4.36x I 0- 8 H), although because the target had very little influence at large displacements,

one would expect them to be identical. This implies that the differences are due to simulation

errors, which cannot be quantified directly since they depend on the particular mesh used for the

solution. None-the-less the difference is less than 5 % and the form of the two- and three­

dimensional result plots are as predicted by the equivalent circuit model.

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oc I 0

4.4

::; 4.2

5

Chapter 3

10 15 20 25

Figure 3.13. The variation of coil inductance, L, with target displacement, d1 for an offset target geometry.

3.4 General Considerations

The FEA simulations of the coil and target system have produced results that compare well with

the experimental observations.

3.4.1 FEA of Experimental Equipment

The simulations discussed above involve idealised models of the coil and target arrangement;

they do not include experimental considerations such as test coils used to measure the field or

spacers used to separate the target and lDS coil.

Test coils

Measurements taken from a system will always affect that system to some extent. In the case of

using test coils to measure the magnetic field, the effect was expected to be negligible since the

coils were stranded and so eddy currents could not form in them. This assumption was

confirmed by completing a two-dimensional simulation of a similar geometry to that of section

§ 3.2.1, but with the incorporation of a test coil. The test coil was modelled as a 5 mm high,

10 mm diameter, empty copper cylinder with an inside diameter of 8 mm, positioned below the

centre of the lDS coil. A plot of the magnetic flux given in figure 3.14(a) revealed no

noticeable change to the field pattern compared to figure 3.3. The magnitude of the z­

component of the magnetic field taken along a line located I mm below the lDS coil is given in

figure 3.14(b) and comparison with figure 3.4 also revealed no significant effect from the

addition of the test coil. These results were taken as justification for neglecting test coils in the

later simulations.

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(a)

Chapter 3

4 ,---------------------------,

": -1------'-~--------==r--~----------l 0

> IO - ; T

JO- GT

J0 - 7 T

< Jo - s T

50 100

R l mm

(b)

150 200

Figure 3.14. Two-dimensional simulation of the lDS coil and target arrangement with a field­measuring test coil. (a) Magnetic flux plot with stronger field represented by lighter colour. (b) Magnitude of the z-component of the field, IB,I I testa, with position R I mm, along a line 1 mm

below the lDS coil.

Plastic Spacers

In the simulations above, the space between the test coi l and the target has been taken as a

vacuum. For the field strengths involved in thi s system, the electrical properties of air were

negligible and so the problem background was modelled as a vacuum. However, for practical

purposes the lDS coil was held above the target using a set of plastic spacers of various heights

to provide an accurate separat ion. It was thought that the non-conducting spacers would not

affect the field since the eddy currents would not form in them. This assumption was confirmed

by completing a two-dimensional simulation based on that described in section § 3.2.1, but with

the incorporation of a plastic spacer. The spacers were machined from clear acrylic block and

the materials catalogue gives the electrical properties of such a material as £, = 3.5000000,

Jlr = 1.0000000, a= 0.0000000 S.m - 1• The width of the block was taken as bei ng that of the

sensor coil and the ax ial-symmetric coordinate system meant that it was modelled as a filled

cylinder positioned directl y below the lDS coil.

A plot of the magnetic flu x given in figure 3.15(a) revealed no noticeable change to the field

pattern compared to figure 3.3. The magnitude of the z-component of the magnetic field taken

along a line positioned 1 mm below the lDS coil is given in figure 3.15 (b) and compari son with

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Chapter 3

figure 3.4 also revealed no significant effect from the addition of the plastic spacers. These

results were taken j ustification for neglecting plastic spacers in the later simulations.

4

r- 3 _r >C

' ::2 --~I

~ 0

0 50 100 150 200

R l mm

(b)

> J0 - 5 T

I0 - 6 T

I0 - 7 T

< I0 - 8 T

(a)

Figure 3.15. Two-dimensional simulation of the lDS coil and target arrangement with a plastic target spacer. (a) Magnetic flux plot with stronger field represented by lighter colour. (b)

Magnitude of the z-component of the field, IB,I I testa, with position RI mm, along a line 1 mm below the lDS coil.

3.4.2 Edge Effects

The edge effect was noticeable through the initial FEA mode ls, for example in fi gure 3.3 where

there is a fold in the flu x above the edge of the target. This is caused by the eddy currents,

which channel the fi eld around the target object. Thi s process is further demonstrated by the

plot of the z-component of the magnetic fi eld shown in fi gure 3. 16.

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Chapter 3

Figure 3.16. Demonstration of the edge effect on the z-component of the magnetic field around the target.

3.4.3 Extraction of Data

The output from the magnetic field sensing test coils and the phase-locking program described

in section § 2.6.2 was a single voltage for the entire area of the coil. This signal was the result

of an averaging effect of the flux passing through the coil. The necessity to compare

experimental and simulation results lead to the requirement for a similar averaging effect to be

applied to the simulated field measurements.

The relationship between the incident field and the output from the test coil is a convolution

of the field pattern as a function of position and the response of the test coil as a function of

position. The convolution operation describes the overlap of two functions, which in this case is

between the magnetic field,f(x, y, z), and the test coil's response g (x, y, z). The convolution of

these two functions at a point, p (X, Y, Z), is given by the integral

f ® g = [!(x,y,z)g(x- X, y -Y,z -Z) dx dy dz (3.29)

This describes the three-dimensional case; in two-dimensions the arrangement is the same but

over the coordinates Rand() (or y and z). In the Maxwell programs, field values were extracted

in a convenient format by taking them from a line by the technique used above (e.g. figure 3.4).

To assist in the process, macros were used to draw the lines at the desired positions and then

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Chapter 3

save the field values to disk. A Java application was constructed to read the data and convolve

them with the coil response function.

For the case of a two-dimensional field solution, lines were constructed to run parallel to the

y-axis (horizontal) over a 5 mm range of 1 mm spaced z-values (vertical). Field values were

taken from the six lines and saved to a series of files with names that described the line

positions. To test the convolution program the coil response was taken as being constant over

the length and width of the coil and coil-field coupling was assumed to be 100 %. The result is

that the coil response function was taken as a step function with fields inside the coil coupling to

the coil and fields outside not coupling to the coil.

In the three-dimensional case, lines were drawn parallel to the y-axis, over a 5 mm range of

1 mm spaced z-values and a 10 mm range of 1 mm spaced x-values. Problem geometries

created by the macro described in section § 3.3.3 produced fields that were symmetrical about

the y-axis. This consideration meant that for test coils positioned on the y-axis, lines only

needed to be drawn on one side of the axis, thereby halving the number of lines to be drawn.

Field values were taken from the 36 lines and again saved to a series of files with suitable

names. As for the two-dimensional convolution, a test was done using a step function to

describe the coupling between the coil and the field.

An example of the three-dimensional convolution is given in figure 3.17, which is the result

of applying the program to the field profile from a small-target simulation. The fluctuations in

the lobes are caused by the edge effect of the target. It can be seen that although the general

pattern in of the filed is unchanged it is smoothed over the area of the test coil. The raw profile

is from a line directly below the centre of the lDS coil, whereas the processed profile takes

contributions from the whole test coil volume. This is responsible for the lower field value in

the central portion of the processed data.

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f-'0

I 0

2

I I I I

~ --- ---- -- - - - -- - , I \ I \ I 1 I 1 I I I I I I I I

0 ~-----=--.---------.---------~~~--~y

- lOO -50 0 50 100

y /mm

Chapter 3

Figure 3.17. Application of the three-dimensional convolution program to the field profile of small­target arrangement. (Solid -) raw field. (Dash --- ) Processed field.

3.5 Summary

In this chapter some of the theory and workings of eddy current FEA have been investigated

and both two- and three-dimensional FEA simulations of an IDS coil and target arrangement

have been developed and refined . The two-dimensional simulations were appropriate for

problems with a large centred target. The three-dimensional simulations were found to take

longer to solve (up to 180 times longer for a solution with a well refined mesh), although they

cou ld be applied to any target and coil arrangement. The models neglected the test coils and the

plastic spacers from the simulations; test simulations were used to justify these assumptions. It

was not possible to quantify the errors on the values produced by the si mulations because the

accuracy of the solution depended on the solver and the nuances of the individual meshes.

Test simulations with d, = 10 mm and w, of three times the IDS coil diameter were completed.

A 2D model was solved with a centred target and a 3D model was solved with Os = 0.5 times the

IDS coil diameter. The simul ations with a refined mesh gave central field values of

2.6 x 10 - 6 T and 2.7 x 10 - 6 T for the 2D and 3D simulations respectively, which were simi lar

in value to the experimentally estimated field strength of- 5 x 10 - 6 T . The coil impedances

were also solved and inductances were found to be 4.051 x 10 - 8 Hand 4.254 x 10 - 8 H for the

2D and 3D cases respectively, which were in agreement with the experimentally estimated

values of- J0 - 7 H. The difference was again due the target offset of the 3D model, which

decreased the coupling and therefore increased the inductance in agreement with the equivalent

circuit models.

Techniques for solving two- and three-dimensional parametric problems have been developed

and were used to demonstrate the influence of target di stance on the impedance of the IDS coil.

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Chapter 3

The results matched the equivalent circuit models and as d, increased (the influence of the target

decreased) L ~ 4.36x 10- 8 H and L ~ 4.58x 10- 8 H for the 2D and 3D models respectively.

Since at large d, the target had little influence on the coil, the differences between the 2D and

3D models must have resulted from differences in the meshes and solvers. A convolution

program has also been developed to match the output from the field simulations and the signal

measured by the test coils. The results have been compared to experimental results and good

correlation was found.

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Chapter 4

Inductive Displacement Sensor Limitations

The first chapter's introduction to IDSs and their limitations provides the groundwork for this

present discussion, which concerns results from a complete investigation of these limitations.

This was achieved using the experimental techniques discussed in chapter two and the FEA

electromagnetic field simulations from chapter three. Firstly, the influence of target material on

the lDS is discussed in section § 4.1 where experiments using aluminium, brass, copper, nickel

and steel are described. The following section (§ 4.2) discusses how displacing the target

laterally relative to the lDS coil affects the reliability of the system. This is closely related to

the final section's investigation of the effect of using targets that are smaller than the

recommended 2.5 - 3 times the lDS coil diameter.

4.1 Target Material

IDSs are usually calibrated in the factory for use with a particular target material and attempting

to measure displacements to different target materials will result in errors. The influence of

target material on the impedance of an lDS coil is described in section § 1.4.1 and equation

( 1.13) shows that coil impedance is not only dependent on target displacement and current

frequency, but also on the conductivity and permeability of the target. To investigate this, the

effect of using different materials on the reliability of IDSs was characterised(§ 4.1.1) and the

results were used to show that the effect was real. Earlier equivalent circuit models of the

system were confirmed by modelling the system with FEA electromagnetic simulations

(§ 4.1.2).

4.1.1 Characterising the Effect of Target Material

An experiment was conducted to characterise the effect of using the lDS to measure the distance

to different target materials. The lDS used for the experiment was calibrated for use with an

aluminium target and it was expected that using it on other target materials would result in

errors in the displacement measured.

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Chapter 4

Table 4.1. Physical properties of some targets investigated.

Sample Width X Thickness I f.lr 0'+ (at 273 Standard Depth of Material Height/mm mm K) /107 Penetration (at 1 MHz) I

±O.Smm ±O.OSmm s -1 .m w-s m

Aluminium 250 X 253 1.50 1.000021 4.00 7.96 Brass 309 X 226 1.30 I 1.59 12.6 Copper 224 X 222 3.30 0.999991 6.45 6.27 Mild Steel 214 X 187 1.00 IOOOt 0.588 0.656 ' Permeability is a function of field 11 = B I H, take I 000 for this estimate. * From Kaye and Laby [39]

Table 4.1 gives the dimensions of the different target samples used in the experiment. The

targets must be of sufficient width to allow eddy currents to flow in the surface as described in

section § 1.4.2. The lDS user manual [10] (p. 15) gives the sensor diameter as 73.7 mm and

since it is unshielded, the target material must be 2.5 - 3 times larger than the sensor. The skin

depth, or standard depth of penetration, was defined in section § 1.2.2 as the point where the

current density has decreased to Ye times its value at the target surface. Table 4.1 gives the

permeability and conductivity, which are used to calculate the skin depth at 1 MHz using the

relation

(4.1)

The distance between the target and the sensor, d1, was varied in 5 mm steps within the range

0- 65 mm. By cycling up and down three readings were recorded and the mean was plotted.

The output voltage was found to vary linearly up to the limit of the sensor range (- 60 mm).

When the target was at a displacement greater than 60 mm the output voltage remained constant.

Figure 4.l(a) shows the displacement to the different target materials as recorded by the lDS.

The axis of abscissas shows the actual target displacement i.e. the physical distance between the

target and lDS barrel. The axis of ordinates shows the target displacement given by the output

voltage of the lDS system. Aluminium was used as the baseline - since the lDS was factory­

calibrated with plate aluminium - hence this plot is linear and the actual target displacement

correspond exactly to the lDS predicted target displacement. From the figure it is apparent that

the mild steel sample gave the most error. The brass and copper sample measurements were in

good agreement with the aluminium.

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6.----------------------------.

> - 4-'5 & ::s 0

Cl 2

0+-----.-----~----~--~----~

10 20 30 40 50 60 Id I 111111

(a)

> g_ g 3.9 Vl 0

40 42

Chapter 4

44 46 48 50 Id I 111111

(b)

Figure 4.1. Influence of target material on lDS displacement measurements. (Solid -) Steel. (Dash --- ) Brass. (Dot ·········· ) Aluminium. (a) Over the whole measurement range. (b) Close-up to

highlight differences.

To highlight the differences between target materials a close-up view for mild steel and

aluminium is given in figure 4.1 (b). Here d1 was varied in 2 mm steps within the range 40 -

50 mm and again, the mean of three readings was found. The two lines have similar gradients

but the steel line is slightly set upwards from the aluminium target. Using linear regression,

expressions describing these straight lines are found to be

Steel: V = 0.087 d 1 -0.049 (4.2)

Aluminium: V =0.091d1 -0.184 (4.3)

each with an R2 value of 0.997. Consider a distance of 10 mm to an aluminium target; this

would produce an output voltage of 0. 726 V. Swapping the target to steel, the same voltage

would correspond to d1 = 9.91 mm, which highlights the problems associated with the influence

of target material.

4.1.2 FEA Simulations of the Influence of Target Material

Using the Ansoft Maxwell 2D program the influence of target material on the magnetic field

was investigated. The two-dimensional module was appropriate because the large centred target

meant that there was axial symmetry. Simulations were completed for each target material at a

range of target distances. The distance between the base of the lDS coil and the top of the target

material was set as a variable that was controlled by the parametric module. The target

materials selected were aluminium, brass, copper and steel as used in the laboratory experiments.

The steel used in the simulations was steel-1008 (plain steel with 0.008 % carbon) which was

chosen because it has similar properties to the sample used in the experiments. A fifth material,

nickel, was also simulated since it does not have a B-H curve (the relative permeability is

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Chapter 4

constant at 600) and it has a conductivity of 1.45 x 10 7 S.m- 1, thus it was quite different to the

other samples and a worthwhile simulation. A suitable nickel target could not be found for the

experimental testing, but it was listed in the Maxwell 20 material catalogue, which

demonstrated the usefulness of the FEA simulations.

In this model there are two primary position coordinates, which were defined thus: z extended

downwards along the vertical axis and was set to be zero at the base of the IDS coil; and r

extended in a horizontal direction from a zero point at the centre of the IDS coil. The distance

between the base of the IDS coil and the top of the target was denoted by d1 and was positioned

at z = dr.

Simulation Results

The complete parametric solutions to the aluminium, brass and copper problems each took

approximately 15 min, whereas the nickel and steel problems each had a much higher solver

time- 200 min. The FEA software required a finer mesh for materials with a high permeability

than for those with a low permeability. This lead to an increase in the processor time that was

required to solve the large number of elements and the large memory usage increased the

processor time required for swapping page files between the virtual and physical memory.

An example of the simulation results is given by figure 4.2, which shows the influence of

target material on iBzi, the magnitude of the z-component of the magnetic field taken along a line

3 mm below the base of the IDS coil (z = 3 mm), for d1 = 15 mm. All the profiles have similar

forms with a high central portion below the IDS coil and an outer lobe. The aluminium, copper

and brass curves lie over each other and appear identical on the given scale, whereas the steel

and nickel profiles are quite different.

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3.E-06 -.--------------------,

E- 2.E-06

= ~.

11 ~

::Q' I.E-06

O.E+OO -l------r----,-----,--~:=;==:':::::::::~

0 20 40 60 80 100 R /mm

Chapter 4

Figure 4.2. Influence of target material on the magnetic field, IBz<z = 3 mm)!, from different target material simulations with d1 = 15 mm. R = 0 mm position is directly below the centre of the lDS

coil. (Dash---) Steel-1008. (Dot .......... ) Nickel. (Solid-) Aluminium, copper, brass.

Steel has the highest central field value, which can be explained in terms of the skin effect.

Equation ( 4.1) shows that the high permeability of steel means that it has a low standard depth

of penetration. This decreases eddy currents in the target material and therefore decreases the

field that opposes the incident lDS coil field. Hence the field below the lDS coil is not

counteracted to the same extent that it is with lower-permeability materials. This is further

illustrated by the plot of central field values given in figure 4.3. With increasing d, the

aluminium and steel curves meet as the influence of the target decreases. But more importantly,

it is noted that the steel target gives a lower spread of central field values, which results from the

skin effect.

3

E-'C --- ---·

I

0 2

= "" 11

'" 0 11 ~ cz:l'

0

0 20 40 60 80

Figure 4.3. Variation in central field value, IBz<r=O, z=3)1, with target displacement, d1• (Dash --- ) §teell-1003. (Dot .......... ) Niclkei. (Solid-) Alumiunium, coppe1r, lln·ass.

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Chapter 4

The influence of target displacement on the IDS coil impedance is shown in figure 4.4. With

increasing target displacement, the resistance decreases and the inductance increases, which is

in agreement with the equivalent circuit equations (1.8) and (1.9). It can be seen that with

nickel and steel targets the effect is substantially different to aluminium, brass and copper.

15.-.------------------------,

3.9 c: 10 :r:

X

0 s 3.7

', "~ ........ 3.5

<:1:: 5

3.3 +-_L_-------,-------------.----------,---'

20 40 60 0 20 40 60 d,lmm d,lmm

(a) (b)

Figure 4.4. Impedance components as a function of target displacement, d1• (Dash --- ) Steel-1 008. (Dot .......... ) Nickel. (Solid-) Aluminium, copper, brass. (a) Resistance, R. (b) Inductance, L.

Edge Effects

The edge effect was introduced in section § 3.4.2 as the channelling of the magnetic flux around

the edge of the target. Interestingly, the strength of the effect depends on the target material and

it is weaker for steel (figure 4.5(a)) than it is for aluminium (figure 4.5(b)). Note that in these

figures, the axis of abscissas starts at R = 35 mm, which corresponds to the edge of the IDS coil,

so these plots only show the external lobes. It might be expected that the higher permeability of

steel would increase the field channelling and thus increase the edge effect, however the higher

permeability also leads to a smaller skin effect and the edge effect is reduced. This effect has

important implications for electromagnetic shielding and is discussed by Marsh and J ohnstone

[40]. The edge effect decreases with target displacement and it was found that in general when

the target was at d, > 30 mm, the edge effect could not be distinguished from the background

field.

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10

f-

' 0 - 5 - I

~

0

35 85 135

Rlmm

(a)

185

f- 7.5 ~

' = 5

<>:i' -2.5

35 85

Chapter 4

135 185

Rlmm

(b)

Figure 4.5. Dependence of edge effect on target material demonstrated by the field plotted along a line 1 mm below the lDS coil. (a) Aluminium. (b) Steel.

Further Investigations

Note from figure 4.2 that the form of the field profiles is the same regardless of the target

material, however the central and outer lobe field values do change. Some further simulations

were completed to investigate this fully and explore whether or not it provides more information

about the target. Since the results for non-ferromagnetic materials were very similar, aluminium

was arbitrarily selected for the further simulations with the assumption that it was also

representative of copper and brass. Models were constructed to find a target displacement

where IB~(r = 0, z = 3)1 matched for both steel and aluminium targets. Since the aluminium

problems were faster to solve, the displacement of aluminium was varied to match the field to

that of existing steel results. Three different values of IBir = 0, z = 3)1 were selected from

previous steel simulations and for each a series of new aluminium results were found to home in

on a target displacement with the same central field value. During each of the simulations

impedance values were also calculated and the results are shown in table 4.2.

Table 4.2. Influence of target material on lDS coil impedance.

IB~(r = 0, z = 3)~/ T Sam~le Material d1 /mm R/10 "n L 110 sH

2.316x 10 Steel-1008 20.0 0.448 3.976 Aluminium 28.2 7.279 3.944

2.405 X 10 6 Steel-1008 25.0 3.685 3.975 Aluminium 32.9 7.211 3.968

2.467x 10 6 Steel-1008 30.0 2.826 4.000 Aluminium 37.8 7.145 4.002

It was found from plots of the results that matching the central field values also matched the

lobe values and so the profiles were identical. This meant that it was only the magnitude of the

field that changed with target displacement and not the shape of the field. This implies that

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Chapter 4

looking at the field profiles in this way cannot provide any more information about the target

material than is already available from the coil impedance.

41.1.3 Target Material Summary

The influence of target material on the output from the IDS has been investigated and it has

been shown that this is a real problem. FEA simulations have been completed for a range of

target displacements to several different target materials. Investigation of the coil impedance

matrix confirmed that the simulations were in agreement with the theoretical equivalent circuit

treatment of the system. Further simulations to match the magnetic field profiles of different

target materials revealed that it is just the magnitude of the field that changes with target

displacement and not the shape of the field. The coil impedance and field are not independent

variables and so this method can not reveal any more information about the target. In summary,

a target-independent IDS cannot be realised by measuring the magnetic field in this way.

4.2 Target Offset

In section § 1.4.3 the influence of target offset on the reliability of inductive eddy current

displacement sensors was introduced. From an empirical point of view, as the target offset

increases one expects the reliability of the IDS to decrease, that is, the target displacement and

output voltage will no longer be linearly related. This section shows how this effect was

investigated; the limitation was characterised experimentally and theoretically (§ 4.2.1), the set

up was modelled with EM FEA simulations (§ 4.2.2) and experiments were used to confirm the

results ( § 4.2.3).

4.2.1 Characterising the Effect of Target Offset

The influence of target offset on the output of an IDS was investigated with an experimental

characterisation. The target material was set at a fixed displacement and the IDS output voltage

was recorded for different lateral displacements. The target displacement was then changed and

a new set of readings was taken.

The target width was fixed at 2.6 times the IDS coil diameter since this is of sufficient size to

avoid the edge effects from too small a target width. The Kaman IDS under test was calibrated

with aluminium and so this was the logical choice for the target material in these experiments.

The results of the previous chapter reveal that the results are similar for materials with a low

permeability and so aluminium is a good representation of copper and brass targets too. The

target was cut from 5 mm thick plate, which is much larger than the skin depth (see table 4.1 ).

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Chapter 4

The thickness also increased the consistency of the results, since it meant that the target was flat

as it did not distort as readily as thinner samples.

The IDS and target were separated by non-conducting spacers and three experiments were

conducted with target displacements of 10, 20 and 30 mm. Figure 4.6 shows the results and

gives the output of the IDS in terms of the percentage error in predicted target displacement.

This is simply defined by

dt(IDS) -dt %distance error= x 100

dl (4.4)

where d1rws1 is the target displacement that corresponds to the recorded IDS output voltage,

whereas d1 is the actual target displacement. The results confirm that the output from the IDS

becomes less reliable as the target offset increases. Note that small errors for d1 = 10 mm at low

offsets are a result of experimental errors where very small changes in voltage lead to a

percentage distance error of - 1 %. As increasing offset leads to the coil and target edges

aligning at - 0.8 times the IDS coil diameter the error becomes large and beyond this point the

readings are highly unreliable. The lower the target displacement, the larger the offset could be

without affecting the IDS output. However, higher target displacements were found to have a

lower error at higher offsets. For offsets larger than those shown in this figure, the curves

reached plateaux when the target no longer has an influence on the IDS.

100

.... 2 75 .... d)

d) u c: r3 50 "' :a

&. 25

0 0 0.4 0.8 1.2

o, I IDS coil diameter

Figure 4.6. Influence of target offset on lDS output. Normalised lDS output with target offset, o., at different target displacements, d1• (Solid -) d1 = 10 mm. (Dash --- ) d1 = 20 mm. (Dot .......... )

d1 = 30 mm

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Chapter 4

4.2.2 FEA Simulations of an Offset Target

The results of the previous section reveal that the IDS coil is affected by target offset, but

further investigations were required to determine the reasons for the effect. FEA simulations

were completed to determine the patterns of the field around the IDS coil. A three-dimensional

geometry was used since the influence of the target on both sides of the IDS coil was of interest

i.e. the influence of the advancing target edge and the receding target edge. Using the

parametric methods described in section § 3.3.3, geometries were constructed with target offsets

os= 0, 5, ... , 150 mm for target displacements d, = 10, 15, ... , 30 mm.

Figure 4.7 shows the influence of large offsets on the field profiles. As the edge of the target

moves below the IDS coil, the magnitude of the field below the coil increases. This is because

the influence of the eddy currents decreases and therefore the IDS coil field is not counteracted

to the same extent as when the target lies directly below the coil.

3 ,------------------------------------,

E- 2 "' I 0

ex:)" 1

o~~~~~~--~----~~~~~

-1.5 -1 -0.5 0 0.5 1.5

y I lDS coil diameter

Figure 4. 7. Field profiles for large offset targets ford, = 10 mm. (Solid --) Os = 0 mm. (Dash---) Os= 100 mm. (Dot .......... ) Os= 100 mm. (Dash dot-·-·) Os= 125 mm. (Dash dot dot_ ... )

Os= 125 mm.

More practical use can be made of the results of smaller offset models as shown by the

example field profiles with offsets Os= 0, 20, 40, 60 mm that are given in figure 4.8. Figures

4.8(a)- 4.8(d) show the field profiles ford,= 10 mm and figures 4.8(e)- 4.8(h) show the field

profiles ford,= 30 mm. Note that the axis of abscissas focuses on the lobe regions and is scaled

in terms of the IDS coil diameter (72 mm) e.g. the edge of the coil corresponds to y = 0.5.

Particular attention should be paid to the variations in the field for the same offset, but different

target displacements. For large target displacements, the d, = 30 mm plot contains just one lobe

that decreases in magnitude with increasing target offset. The peak of the lobe remains at the

79

L________________________________________________________________ -- -

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Chapter 4

same position, independent of the offset. However, the d, = 10 mm field includes three lobes

and the middle lobe is drawn to the left as the target edge advances. The difference between the

d, = 10 mm and d, = 30 mm field profiles is a result of the target edge effect, which was

discussed in section 3.4.2.

Os! d1 = lOmm d1 =30mm mm

12 12

,.... 8

,.... 8

' ' 0 0 - -- -0 ~4 ~4

0 0 0.4 1.6 2.2 2.8 0.4 1.6 2.2 2.8

y I lDS coil diameter y I lDS coil diameter

(a) (e) 12 12

,.... 8

,.... 8

~

' ' 0 0

~ - -- -

20 ~4 ~4

0 0 0.4 1.6 2.2 2.8 0.4 1.6 2.2 2.8

y I lDS coil diameter y I lDS coil diameter

(b) (f) 12 12

,.... ~

8 ,....

8 ' ' :::: 0 - -- -

40 ~4 ~4

0 0 0.4 1.6 2.2 2.8 0.4 1.6 2.2 2.8

v I lDS coil diameter v I lDS coil diameter

(c) (g)

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12,--------------------------~

:-- 8

60 ~:~l/~ 0.4 1.6 2.2 2.8

y liDS coil diameter

(d)

Chapter 4

12,--------------------------~

:-- 8 ' 0

~4

~ 0~--~----~==~====~

0.4 1.6 2.2 2.8

y liDS coil diameter

(h)

Figure 4.8. FEA simulations of offset targets at different target displacements. (a)- (d) d1 = 10 mm. (e)- (h) d1 = 30 mm.

Figure 4.9 shows the influence of target offset on the lDS coil inductance for different target

displacements. With increasing offset, the curves converge to a point as the influence of the

target diminishes. These results are in agreement with the equivalent circuit model described by

equation ( 1. 9), which shows that closer targets result in a lower lDS coil inductance because of

the stronger coupling to the target.

00

I

4.5 .--------------------------------------------.,

0 4.25

4+-----------,-----------,-----------~

0 0.4 0.8 1.2 os I IDS coil diamater

Figure 4.9. Influence of target offset on coil inductance. (Solid -) d1 = 10 mm. (Dash --- ) d1 = 20 mm. (Dot ·········· ) d1 = 30 mm

Figure 4.10 shows the change in coil impedance and lobe amplitude with target offset. Recall

that the lDS measures target displacement only using the coil impedance.

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Chapter 4

.--------------------,- 4.44

4.4 ;--6

I

0

:r: oc

I

4.36 0

-l

4.32

2 +---,,-------,---,---,-------,--....,---'- 4.28

0 0.2 0.4 0.6 0.8 1.2

Offset I IDS coil diameter

Figure 4.10. lDS coil impedance and magnetic field lobe amplitude for d1 = 30 mm. (Left, solid -) Lobe amplitude. (Right, broken --- ) IDS coil inductance.

4.2.3 Experimental Measurements of an Offset Target

The results of the previous section were confirmed by experimentally measuring the output

from the lDS taking test coil readings at the same time. For d1 = 25 mm and with a target width

of 3.3 times the lDS coil diameter, the target was offset and readings taken. The results are

given in figure 4.11, with the test coil output scaled such that a value of I corresponds to the

reading with no offset and the lDS output scaled to give the percentage distance error.

.... 5. :; 0

:g 0.8 u .... "' 2

"0 0.6 V

"' ~ § 0.4 z ---0.2 -!""-'~"--;.---'"""-=r-=-=-o...:-=-=j-'-=_"-'_=-=_'--'_T--_--,-----,-------'-

0 0.2 0.4 0.6 0.8 1.2

Normalised sensor coil offset

12

10

..... 8 0

!:: 0)

0)

6 u c: .:s "' :a

<>'<

2

0

Figure 4.11. Experimental confirmation of FEA simulation results. (Left, solid -) Normalised test coil signal. (Right, broken --- ) lDS distance error.

4.2.4 Target Offset Summary

The influence of target offset on the output of the lDS has been characterised and was shown to

be a real problem that leads to a decrease in reliability of the measurements from the system.

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Chapter 4

The lower the target displacement, the larger the offset could be without affecting the IDS

output. However, higher target displacements were found to have a lower error at higher offsets.

FEA simulations were conducted and the results were found to agree with experimental

measurements. It is proposed that by using an array of small test coils around the IDS it would

be possible to compensate for the influence of target offset on the IDS output. The relationship

between the lobe shape and amplitude is not trivial and either a look-up table or a trained

artificial neural network could be utilised to convert test coil measurements into an IDS

correction factor. In this way, the influence of target offset on the output from an IDS could be

corrected, which would result in more reliable displacement measurements.

4.3 Target Width

The influence of target width on the output from an IDS was introduced in section § 1.4.2 and is

closely related to target offset. In this section the effect of using targets smaller than the

recommended width is investigated, which begins with a characterisation of the effect in section

§ 4.3.1, where it is shown that the problem is real and the resulting measurement errors are

calculated. The results of FEA simulations are presented in § 4.3.2 and conclusions are drawn

in section § 4.3.3.

4.3.1 Characterising the Effect of Target Width

The influence of target width on the output from the IDS was characterised experimentally. As

in the previous section, aluminium plate targets with a thickness of 5 mm were used since the

IDS was factory-calibrated for this material; the thickness targets ensured a flat surface for the

experiment. Two experiments were completed: the first measured influence of target size on the

IDS output voltage for a fixed target displacement; the second concerned using the IDS to

measure the displacements to different target widths. For both experiments, target

displacements were controlled with non-conducting plastic spacers.

The target was maintained at a constant displacement, d1 = 20 mm and the output from the

IDS was measured with different target widths. The targets used in the experiment were as

follows: 2.6, 2.4, ... , 1.2, 1.0 times the IDS coil width. As the effects were observed to increase

sharply as the target size approached the diameter of the IDS coil, an additional target was

constructed with a width of 1.1 times the IDS coil width. Figure 4.12 shows the results from the

experiment, from which it can be seen that as the target width increases, the accuracy of the IDS

increases. The curve levels out, which shows that using a target wider than about 2.5 times the

IDS coil diameter does not improve the IDS accuracy.

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1.75 > '5 %1.65 0

r/J

e 1.55

1.5 2 2.5

W 1 I IDS coil diameter

Figure 4.12. Influence of target width on the lDS output.

Chapter 4

In the next experiment, three target sizes were investigated: 2.6, 1.4 and 1.2 times the IDS

coil width. For each target, the output from the IDS was measured at different target

displacements. The results are shown in figure 4.13, from which it can again be seen that the

IDS reliability deteriorates with decreasing target width. Figure 4.13(a) shows that the linearity

of the system is dependent on the target width and displacement. Smaller targets give reliable

results at lower target displacements and it is only when the target is moved further away that

the output deviates from a linear response. By comparing the measured voltage with the output

that would be expected at a given target displacement, a measure of distance error can be

obtained, which is defined by equation (4.4). This error is plotted for target displacements

larger than 25 mm in figure 4.13(b ).

6 30

5 25 > 4 -5 3 & :::l

2 0

"' 9 I

:s po V

~ 15

~ 10 ~

0 5

-I 0 0 10 20 30 40 50 25 30 35 40 45 50

d 1 1mm d, /mm

(a) (b)

Figure 4.13. Influence of target width on the lDS output. (Solid -) w, = 2.6. (Dash --- ) w1 = 1.4. (Dot··········) w, = 1.2. (a) Non-linearity introduced with different target widths. (b) Distance

measurement error resulting from small target widths.

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Chapter 4

4.3.2 FEA Simulations of the Effect of Target Width

Using Ansoft's Maxwell 3D program, the influence of an offset target on the field around the

lDS was investigated. The three-dimensional module was selected because as the width of the

target decreased, the influence of the corners increased and so the approximation that the target

was axially symmetric -as had to be assumed in two-dimensional simulations -increased the

modelling error to an unacceptable level. Two groups of simulations were run: one with

d1 = 10 mm and another with d1 = 20 mm. For each group, nine simulations were run with each

having a different target width.

Some results from the FEA simulations are presented m figure 4.14, which shows the

influence of target width on the field profiles. Figures 4.14(a) -4.14(c) are for a target

displacement of d1 = 10 mm and figures 4.14( d) - 4.14( e) are for a target displacement of

d1 = 20 mm. Comparing these figures with figure 4.7, highlights the difference between the

influences of target offset and target width. As has been explained in previous sections, the

central portion of the field, below the lDS coil, is reduced in magnitude for a lower target

displacement. The influence of an offset target is to skew this central portion, whereas a small

target width gives a skewed effect for both sides and the result is a central dip. This is less

prominent at higher target displacements, which indicates that it results from the edge effect that

was described in section § 3.4.2.

The influence of a small target width on the outer lobes is similar to that observed for an

offset target. At small target displacements, the edge effect causes the outer lobes to be broken

into separate lobes. However at large target displacements, this effect is not present and there is

a single lobe that decreases in magnitude with decreasing target width.

W 1 f IDS dia

15

f-

'7 10 0

2.6 cci' 5

d1 = 10 mm

0+-~~--~--------~---r~~

-1.5 -I -0.5 0 0.5 1.5 y I lDS coil diamter

(a)

d1 =20mm

15

f-,_ 10 I

s --cci' 5

0

-1.5 -I -0.5 0 0.5 1.5 y I lDS coil diamter

(d)

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Chapter 4

15 15

f- f-~

10 ~

10 ' ' 0 = - -- -1.8 ~, 5 ~5

0 0

-1.5 -1 -0.5 0 0.5 1.5 -1.5 -1 -0.5 0 0.5 y I lDS coil diamter y I lDS coil diamter

(b) (e)

15 15

f- f-';- 10

~

10 '

= 0

- -- -1.0 ~- 5 ~5

0 0

-1.5 -1 -0.5 0 0.5 1.5 -1.5 -1 -0.5 0 0.5 y I lDS coil diamter y I lDS coil diamter

(c) (f)

Figure 4.14. FEA simulations of the influence of target width on the magnetic field. (a)- (d) d1 = 10 mm. (e)- (h) d1 = 20 mm.

4.3.3 Target Width Summary

1.5

1.5

The use of small targets on the output from IDSs has been characterised and it was shown that

there is a real effect on the reliability of the distance measurements. The effect is similar to that

of an offset target and at low displacements the target affects the lobe shape. A similar array of

test coils that was proposed to measure an offset target could also be used to counter the

influence of target width.

4.4 Summary

In this chapter the techniques developed previously were applied to investigate the limitations of

IDSs. The test coil design that was described in chapter two was applied to measure the field

around the test coils experimentally and the FEA methods discussed in chapter three have been

utilised to simulate these fields. A combination of two- and three-dimensional FEA simulations

have been used to investigate the influence on the lDS output of target material, target offset

and target width.

The effect of target material on the lDS was demonstrated by obtaining two equations for the

measured voltages and the corresponding target displacement: for steel V= 0.087d,- 0.049 and

for aluminium V= 0.091 d, - 0.184, each with an R2 value of 0.997. Solutions for steel and

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Chapter 4

nickel problems took approximately 13 times longer than aluminium, brass and copper targets.

The field profiles for aluminium, brass and copper overlapped and with d1 = 5 mm, the

iBz(r = 0, z = 3)1 values were 3.07 X 10- 7 T. The values were 6.15 X 10- 7 T and 1.49 X 10- 6 T

for nickel and steel respectively. The difference resulted from reduced coupling to the higher

permeability materials, which is a consequence of the skin effect. As d1 - oo and the influence

of the target material decreased, the central field values all tended to the same value of

2.53 x 10- 6 T. Further simulations showed the edge effect was stronger for an aluminium

target than a steel target. The impedance results were observed to follow the equivalent circuit

models. Further steel and aluminium simulations were ran to match the central field values.

This was also found to match the lobe amplitudes and so it was determined that monitoring the

lobes did not reveal more information about the target material.

The influence of an offset target on the reliability of an IDS was investigated experimentally

and with FEA simulations. An experimental characterisation of the influence of offset revealed

that the lower the target displacement, the larger the offset could be without affecting the IDS

output, but conversely that higher target displacements yield a lower error at higher offsets. For

example with os= 1.23 times the IDS coil diameter the distance errors were 107, 70, 58% for

d1 = 10, 20, 30 mm respectively. FEA investigations showed that the impedance of the IDS coil

followed the behaviour described by the equivalent circuit equations. The value of the

simulated impedance with the target at a large offset was approximately 20% larger than for the

same experiment conducted in 2D for the material investigation.

The target edge effect was found to play an important part in shaping the lobes at low target

displacements. At low target displacements the field external to the IDS was found to comprise

a number of distinct sub-lobes, whereas at higher target displacements only a single lobe was

found. By monitoring the lobe amplitudes with a test coil array it was found that the effect of

an offset target could be corrected. For example, with d1 = 25 mm and W 1 = 3.3 times the IDS

coil diameter, when Os= 1.2 times the IDS coil diameter the distance error was 3.6 %, which

corresponded to a normalised test coil output of 0.54.

The influence of target width on the IDS was demonstrated to be similar to that of target

offset and edge effects were again important at low target displacements. It was proposed that

the lobes could be monitored using an array of test coils and either a look-up table or an

artificial neural network could used to compensate for the affects of target offset.

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Chapter 5

Conclusions

The primary aim of the work described in this thesis was to investigate the limitations of

inductive proximity sensors and it was initially proposed that measuring the field external to an

IDS could provide more information than was available from the lDS coil impedance alone.

The first chapter included a general discussion about displacement sensing and applications

where different technologies are appropriate. Particular emphasis was placed on comparing

behaviour in harsh environments where dust, dirt, oil, humidity, etc. can interfere with the

measuring process. This discussion lead to the confirmation that IDSs were suitable for making

displacement measurements in harsh industrial environments and that they had advantages over

other technologies that could not perform as well in these conditions. The discussion of lDS

operating principles lead to an understanding of their limitations and it was shown that target

material, offset and width affected the sensors. IDSs have been widely used in industry for a

number of years and many systems are available commercially, consequently it was determined

that an investigation of their limitations was an important physical problem.

The field around the IDS coil was found to be sinusoidal with a magnitude - I 0- 6 T and a

frequency of I MHz. A comparison of magnetic sensing technologies in the second chapter

determined that a number of devices are available that can measure a field with these

characteristics although many - such as SQUIDs - would be impractical for the application

environment. A simple test coil was shown to be the most appropriate device for this

application, although a phase locking signal processing technique was required to produce a

high signal to noise ratio at low field strengths ( < 2 x 10- 6 T). Before processing, an example

signal was found to have a mean amplitude of 4.65 x 10- 4 V with a variance of 4.36 x 10- 7 V2,

but the phase-locking technique revealed an amplitude of 0.0324 V with a variance of

l.I2 x 10- 7 V2. Hence a system was developed that could reliably measure the magnetic field

around the lDS coil.

The third chapter described work to simulate the magnetic fields around IDSs with

commercial FEA software. Both two- and three-dimensional models were constructed, tested

and refined to produce smooth field values. Central field values produced by the 20 and 3D

models were 2.6 x 10- 6 T and 2.7 x 10- 6 T respectively, which matched the experimentally

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Chapter 5

measured value of- 5 x 10- 6 T. Also, investigation of the influence of target displacement on

the impedance of the lDS coil found the behaviour to match with the equivalent circuit models.

Hence the simulations were shown to be an accurate model of the experimental equipment. A

program, that was developed to convolve the simulated field and test coil response, was found

to improve the match between experimental and simulation results and the result was a system

suitable for the investigation of limitations of lDS systems.

The effect of target material was shown to be real experimentally by calibrating the lDS,

which was demonstrated by the two relations: V= 0.087d1 - 0.049 (for steel) and V= 0.09ld1 -

0.184 (for aluminium), each with an R2 value of 0.997. Simulations were setup that produced

impedance values that agreed with theoretical models. These simulations showed that the field

profiles of aluminium, brass and copper were very similar and when d1 = 5 mm, the

IBzCr = 0, z = 3)1 values were 3.07 x I 0- 7 T. For nickel and steel, the values were 6.15 x 10- 7 T

and 1.49 x 10- 6 T respectively. This demonstrated how the permeability of the target material

affected the lDS field. Further simulations were completed to investigate this further and it was

found that varying d1 to match the central field values also matched the lobe amplitudes. This

meant that it was not possible to reduce the target dependence by monitoring the field in this

way.

The target offset effect was demonstrated experimentally by measuring the distance error with

offset. For example when Os= 1.2 times the lDS coil diameter, the distance errors were 107, 70,

58% for d1 = 10, 20, 30 mm respectively. This showed that the target offset effect was a real

problem that could potentially have made measurements highly unreliable. FEA simulations

revealed the effect of the offset targets on the magnetic field around the lDS. Agreement was

found between the simulated and theoretical coil impedance variations, which confirmed the

appropriateness of the model. The external field lobe on the side nearest the leading offset edge

was affected while the trailing edge was unaffected. Two key features in the leading edge lobes

were observed: the amplitudes decreased with increasing offset and at low target displacements

the edge effect caused the lobes to split. An experiment with the test coil array confirmed that it

was possible to use the change in lobe amplitude to measure the offset of the target, for example

when d1 = 25 mm and w 1 = 3.3times the lDS coil diameter, with Os= 1.2 times the lDS coil

diameter the distance error was 3.6 %, which corresponded to a normalised test coil output of

0.54. Hence it was possible to correct the output signal from the lDS coil to counteract the

effect of an offset target.

Target width was found to have a similar effect to target offset. Again, experiments were

completed which showed that the effect was a real problem, for example with d1 = 20 mm when

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Chapter 5

w1 = 1.2 times the lDS coil diameter, the output was 8 % larger than it was when w1 = 2.5. FEA

simulations showed that both sides of the lDS external field lobes were affected by the smaller

target compared to just one side with an offset target. The same features were observed in the

field lobes: the amplitudes decreased with increasing offset and at low target displacements the

edge effect caused the lobes to split. Hence it was possible to measure the lobe amplitudes and

correct the lDS output to compensate for the target width effect.

Future work could develop the test coils further and produce an array suitable for use in harsh

environment applications. Also, the target offset and width corrections could be developed with

the use of either look-up tables or artificial neural networks to utilise the lobe splitting that was

caused by the edge effects.

The macros and the convolution program were very versatile and future work could utilise

them as they could easily be adapted to use new geometries and materials. The experiments for

the effect of target offset and width only looked at aluminium targets, which were taken to be

representative of targets with a low permeability. Steel targets were not simulated because of

the time taken to produce solutions, which was a consequence of the large mesh sizes. Future

work could complete these experiments on a more powerful computer. A further parameter that

could be investigated is target thickness; simulations could be run to see the effect of using

targets approaching the skin depth. This could also be achieved by modifying the macros.

The frequency of the lDS coil that was simulated was fixed, however the skin effect was

dependent on the frequency of the exciting radiation and so simulations involving different

frequencies or a burst of frequencies would be worthwhile.

When measuring the magnetic fields, only the magnitude of the test coil signal was measured.

In practical experiments phase information was lost in the signal processing program and in the

FEA simulations the phase information was not collected by the macros and convolution

program. Further work could investigate the effect of the parameters on the phase of the test

coil signal.

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Appendix 1

Published Research

The paper "Improving the Reliability of Eddy Current Distance Measurements with Finite

Element Modelling" by M. R. Wilkinson and S. Johnstone was taken to The Institute of Physics

Sensors and their Applications XII conference in Limerick, Republic of Ireland in September

2003. It is published in the book Sensors and their Applications XII (0750309748) by Institute

of Physics Publishing in 2003. It is reprinted here with permission.

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Appendix 1

IImm JP) Jr@ vnlillg lllhl ~ IRtellnSllbl iillii lly @it' IE<dl dl y CC unJrlrtelillll JI))Ji§lt311ill <e~ M~Sl§lilllr~m~lillll§ wnlllhl IFniDliillte IEllem~Il1lll M@dl~llllniDlg

M. R. Wilkinson, S. Johnstone

School of Engineering, University of Durham, South Road, Durham, DH1 3LE, United Kingdom

Abstract: Eddy current distance measuring devices are used widely in a number of harsh environment applications. However they have limitations and this paper looks at the effect of non-centred targets on the reliability of such devices. It was found that when a target was offset by 1.3 times the sensor coil diameter there was an error of 6.5% in the distance measured.

Finite element electromagnetic field simulations have been employed to model the system and have shown how the field outside the sensor coil changes with target offset. By monitoring this field with small test coils it is possible to correct the distance measurement error. This work has potential to lead to an improvement to the range of applications in which eddy current distance measuring devices may be employed.

1. ][ntrodu.nction

Eddy current sensors (ECSs) [1] are widely employed to measure the distance to conducting targets in harsh environments [2]. Such true position measuring devices comprise a sensor coil and associated electronics. An alternating current is passed through the coil to generate an electromagnetic field. When a conducting target material is placed in this field, eddy currents are generated which produce an opposing field thus reducing the original intensity. This causes an impedance variation in the sensor coil which is detected by the monitoring electronics. The distance to the target is given as a voltage that is directly proportional to the target displacement. Non conducting materials between the ECS and target will not affect the field and so they can operate in environments where dust, oil or humidity, etc. are present. This is a major advantage over other distance measuring devices.

The distance range over which an ECS will provide linear results is directly proportional to the diameter of the ECS coil. The magnetic field around ECSs with a shield is less extended than for unshielded designs. This has the effect of reducing the measuring range, but means that smaller targets may be used. For shielded ECSs the target size should be at least 1.5 to 2 times the ECS coil diameter and for unshielded ECSs the target should be at least 2.5 to 3 times the ECS coil diameter [3]. Using a target size smaller than these limits reduces the linearity and long term stability. A similar effect is observed when the target is offset from centre; that is the target extends a greater distance on one size of the ECS coil than on the other. Previous authors have looked at various aspects of ECS reliability [4, 5], but this paper summarises research into a solution to the offset problem and is a subset of wider work on the limitations of ECSs.

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Appendix 1

Experimental work was carried out using a commercially available eddy current distance measuring device from Kaman Instrumentation. This enabled the researchers to avoid the complication of constructing and fine-tuning such a device [6] and meant that the limitations of a well calibrated system were investigated. The system was modelled using Ansoft's Maxwell3D™ finite element electromagnetic field solver using an eddy current module; this is detailed in section two. The results of these simulations have been confirmed experimentally (section three) and section four shows how they were interpreted and exploited.

2. Simulation of Target Offset

There are a number of modelling methods through which more can be learnt about electromagnetic sensor designs. Early analytical work on shielding and eddy current problems [7, 8] is relevant but limited to simple geometries. Probable flux methods [9] are suitable for complex geometries, but often require large assumptions. However with increasing computing power rigorous numerical finite element methods [ 10, 11] have proven to be useful in three dimensional and high frequency cases [12].

The ECS coil was modelled as a 1 mm wide rectangle swept 360° around a central axis with an alternating current source running at 1 MHz. The magnetic field strength was measured below the ECS coil using a test coil. By treating it as a solenoid, the amplitude of the current in the coil was estimated. This value was then adjusted so that the simulated field strength matched the measured field strength. The ECS coil was located above a square aluminium target that was positioned with various offsets relative to the ECS coil as illustrated in figures 1 (a) and 1 (b). The target material had a width of 3 times the ECS coil diameter and a thickness of 5 mm. The distance between the ECS coil and the target was fixed at 20 mm.

Finite element field solutions were computed on a fine mesh and the magnitude of the magnetic field in the direction along the ECS coil axis (z-axis in figure 1), IBzl, was measured on a line perpendicular to the ECS coil axis (y-axis in figure 1) in the region between the ECS coil and target.

--+-+-'Y

r . r dLY~

r ! r ITL~~

====

(a) (b)

Figure 1. Wire frame perspectives of the problem geometry for (a) a target offset of zero and (b) a target offset of 0.6 times the sensor coil diameter.

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l.SE-06

1-.::; l.OE-06 ~

S.OE-07

-1.5 -1 -0.5 0 0.5 1.5 Position I ECS coil diameter

(a)

Appendix 1

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1.5E-06

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5.0E-07

O.OE+OO +. ----,-----'T----.-~r"---"--,.----1

-1.5 -1 -0.5 0 0.5 1.5 Position I ECS coil diameter

(b)

Figure 2. The field profiles for (a) a target offset of zero and (b) a target offset of 0.6 times the sensor coil diameter.

The field was found to consist of a higher central portion immediately below the ECS coil and two 'lobes' to either side. As the offset was increased (i.e. the ECS coil was displaced laterally relative to the target centre) the lobe on the side closest to the advancing target edge decreased in magnitude and was curtailed in its lateral extension. This is illustrated in figure 2 which shows the field patterns for an offset of zero and an offset of 0.6 times the ECS coil diameter.

''''''"' \\\ ,,,, \\'\\'-.'-.\\' \\\} ~\ ZL '\'\\\\\'-\ ~111 \\\\\\\\ 11\\

\\\\\\\\11)1111 1\\\\11111 I 11 \ I I l I I 1. I I I I. I I I I Y l.l!IJil!.JIIIfllllll,l·l· ... I. I f I I I I I I I I I I I / ll!llllllilllllt!il// llil!lll/;//;till//// il//ll/11////lll///// ///////1////////----~ ////////////// ..... -~-----~---·

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. \('\'\\\\\\\\\\\\ \1\l\\111\\\\ll \ I \1 I I l I I I. I I \ l

I I I I I I I I I I I 11. I I I Y ) f f ) f I I. I I I I I ';' I I I I 1 I I I. I I I I, I I I I I I I I /. I I I I I I I i 1 1 I r1 I!;/ 1 /; 1 1 I 1 1 /1 I 1 I //!ll////1//1/11/;/111 //1////////////1////// ////////////////////// //////////..-"..-"//..-"/////// /~/?~~~~~~~~~~~~~///~/

(b)

Figure 3. Direction of the magnetic field for a given phase angle on the y-z plane cross section through the ECS coil, target and profile line for (a) a target offset of zero and (b) a target offset of 0.6 times the sensor coil diameter. Note that the magnitude of the field

is not shown by this diagram.

The form of the field profiles may be understood in terms of the direction of the magnetic field vectors as illustrated by figures 3(a) and 3(b). Below the centre of the ECS coil the vectors are vertical (large z-component) as they are within the coil. Moving along the profile line away from the ECS coil centre the flux lines start to curve around and the vector takes on an increasing horizontal component. Immediately below the ECS coil edge the vector is horizontal (large y-component) and the there is a dip on the curves of figures 2(a) and 2(b). For the zero-offset geometry the z-component of the field increases as the flux lines sweep back up to join the upper end of the ECS coil. IBzl then drops off as the field decays with increasing displacement from the source. For the

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Appendix 1

geometry with an offset of 0.6 times the ECS coil diameter there is also an initial increase as the flux sweeps back up, however in this case the target edge comes into play. Some of the flux lines are swept down and around the target so the field lines are spilt. This has the effect of creating more horizontal than vertical components of the field and thus IBzl decreases.

3. Experimental Confirmation

The modelling results were confirmed by measuring the magnetic field outside of the ECS coil with small tightly-wound test coils. These test coils were constructed from fine copper wire and an air core was used so as to minimise the disruption to the field. The stranded nature of the devices meant that eddy current interactions were small. An Agilent Technologies impedance analyser was used to match the natural frequency of the test coils closely to the 1 MHz of the ECS coil; this enabled maximum response and sensitivity. The test coils were connected to a digital oscilloscope and the amplitude of the signal recorded.

Two test coils were employed and were positioned either side of the ECS coil on the y-axis in figure 1 so as so track changes in the lobes of figure 2. The offset of the target material was increased and the output from the test coils was recorded. This has been expressed in normalised terms to highlight the variation from the zero-offset case. The ECS output was also recorded and was observed to change as the offset increased, even thought the actual target distance (d1) remained constant. This is expressed in terms of a percentage distance error, which is simply:

dr(en) -dr % distance error = · x 100

dr

where dt(ecs) is the distance given by the eddy current ECS. Figure 4 shows the normalised output of the test coil on the side of the

approaching target edge (i.e. positive y-axis position on figure 1) and the % distance error. For low values of the normalised ECS coil offset (:S0.6), the small distance errors were caused by experimental limitations and were not actual device errors.

'[ Test coil :; 0

~ 0.8 (.) ~ [/)

~ -o 0.6

<1)

.~ C<i E Ci 0.4 z

Distance error ---0.2 i=-'='--'=;-~=-r=-=-:-=-=-=--=-::;-=--=-=-=-=-::r-'----,---~----'-

0 0.2 0.4 0.6 0.8 1.2 Normalised sensor coil offset

12

10

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<1)

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2

0

Figure 4. Graph showing percentage distance error resulting from target lateral displacement and the output from the test coil.

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Appendix 1

When the ECS coil and target edges were aligned (an offset of 1 times the ECS diameter) there was a 6.5% error in the target distance as given by the ECS. The output of a test coil positioned at 1.3 times the ECS coil radius was found to be 0.47 of the value when the target was centred. Thus by monitoring the test coils in this way, it was possible to correct for the errors caused by target offset.

The direction of the target offset was also determined by comparing the output from the two test coils. As can be seen in figure 2 only the lobe closest to the approaching target edge was affected; the opposite lobe remained static.

4. Condusions

This paper has demonstrated by using finite element field simulations that there is more information available from the ECS system than is extracted by only measuring the impedance of the ECS coil. Outside the ECS coil lobes were observed in the z­component of the magnitude of the magnetic field. As the offset of the target material was increased the lobe on the side of the advancing target edge was observed to decrease in magnitude and its lateral extension was curtailed. By monitoring small test coils positioned to observe these lobes it was possible to counteract the effect on the ECS coil.

With further work the system of test coils and the ECS coil could be combined into a package that was resistant the harsh environment in which ECSs are often employed. The signal from the test coil could be monitored by an electronic system that could directly modify the output from the ECS device. This would make an eddy current distance measuring device that could be used in situations where the target materials were not always centred. Such applications include environments targets move through the path of the ECS (e.g. production lines) and where the target may be knocked out of alignment (e.g. rolling mills).

Acknowledgements

This work is supported by funding from the UK EPSRC reference number GR/R58475/0l.

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Appendix I

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